<TABLE BORDER>
<TR>
<TH>PI</TH><TH>Institute</TH><TH>Proposal</TH></TR>
<TR><TH>Aalto S.</TH><TH>
Steward Observatory, University of Arizona </TH><TH>
Centre and Disk Spectroscopy of Interacting Galaxies </TH><TR><TH>
Abergel A.</TH><TH>
Institut D'Astrophysique Spatiale - Orsay </TH><TH>
Very Cold Dust Imaging </TH><TR><TH>
Alcolea J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
Dust Distribution around Bipolar PPNEE </TH><TR><TH>
Allamandola L.</TH><TH>
NASA/Ames Research Center - Moffett Field </TH><TH>
Specific PAH and Amorphous Carbon Structures </TH><TR><TH>
Allamandola L.</TH><TH>
NASA/Ames Research Center - Moffett Field </TH><TH>
The D/H Ratio in Interstellar PAHs the Search for Interstellar Pads</TH><TR><TH>
Andre P.</TH><TH>
Service d'Astrophysique-Saclay, Gif Sur Yvette </TH><TH>
Magnetic Field Geometry Toward Embedded Outflow Sources </TH><TR><TH>
Andre P.</TH><TH>
Service d'Astrophysique-Saclay, Gif Sur Yvette </TH><TH>
Spatial Structure of the Youngest Protostars An Absorption Study</TH><TR><TH>
Andreani P.</TH><TH>
Dipartimento Di Astronomia, Univ. Padova </TH><TH>
FIR Photometry of a Complete Sample of Optically Selected Bright Quasars.</TH><TR><TH>
Andreani P.</TH><TH>
Dipartimento Astronomia, Univ. Padova </TH><TH>
Spectrophotometry of a Complete Sample of IRAS Galaxies With
Millimetric Fluxes, CO and HI Data.</TH><TR><TH>
Antonucci R.</TH><TH>
University of California at Santa Barbara </TH><TH>
Search for CO Absorption in the Cygnus A Torus </TH><TR><TH>
Appenzeller I.</TH><TH>
Landessternwarte Heidelberg </TH><TH>
Using IR Coronal-Lines As Calorimeters for AGN </TH><TR><TH>
Appleton P.</TH><TH>
Iowa State University - Ames </TH><TH>
IR Imaging of Collisional Ring Galaxies </TH><TR><TH>
Arendt R.</TH><TH>
Applied Research Corp. - Greenbelt </TH><TH>
Unusual Line and Continuum Emission in the Cas A SNR </TH><TR><TH>
Armus L.</TH><TH>
California Institute of Technology - Pasadena </TH><TH>
The Far Infrared Spectral Energy Distribtions of High Redshift Quasars</TH><TR><TH>
Axon D.</TH><TH>
Nuffield Radio Astronomy Lab - Macclesfield </TH><TH>
The Kinematics and Physical Structure of Molecular Tori </TH><TR><TH>
Bachiller R.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
Molecular IR Lines As Tracers of Infall and Outflow in Star Forming Cores</TH><TR><TH>
Bachiller R.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
The Bipolar Outflows From the Youngest Stellar Objects Infrared Spectroscopy</TH><TR><TH>
Bania T.</TH><TH>
Department of Astronomy, Boston University </TH><TH>
Probing the Structure of Nearby Translucent Molecular Clouds </TH><TR><TH>
Bania T.</TH><TH>
Department of Astronomy, Boston University </TH><TH>
Probing the Structure of the Nearest Molecular Cloud MBM-12 </TH><TR><TH>
Barbieri C.</TH><TH>
Universita` di Padova, Dip. di Astronomia - Padova </TH><TH>
IR Observations of Rosetta Asteroidal Targets. </TH><TR><TH>
Barlow M.</TH><TH>
Dept. of Physics and Astronomy, UCL, London </TH><TH>
Photometry of a New Sample of candidate Vega-Excess Sources </TH><TR><TH>
Barlow M.</TH><TH>
Dept. of Physics and Astronomy, UCL, London </TH><TH>
TOO: Observations of Novae During the ISO Mission </TH><TR><TH>
Barr P.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Infrared Observations of Cygnus X-3 </TH><TR><TH>
Barr P.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
ISO Observations of the Egret Blazars </TH><TR><TH>
Barrado Navascues D.</TH><TH>
Depto. Astrofisica, Universidad Complutense - Madrid </TH><TH>
The Infrared Spectrum of Chromospherically Active Stars </TH><TR><TH>
Barthel P.</TH><TH>
Kapteyn Astronomical Institute - Groningen </TH><TH>
The Nature of Broad Line Radio Galaxies </TH><TR><TH>
Barucci A.</TH><TH>
Observatoire De Paris-Meudon </TH><TH>
Dark, Volatile-Rich Asteroids: Possible Relation to Comets. </TH><TR><TH>
Barvainis R.</TH><TH>
MIT Haystack Observatory - Westford </TH><TH>
H2 Emission from the Molecular Torus in Cygnus A </TH><TR><TH>
Barvainis R.</TH><TH>
MIT Haystack Observatory - Westford </TH><TH>
ISO Observations of the Cloverleaf, a Quasar with CO at Z=2.5 </TH><TR><TH>
Baudry A.</TH><TH>
Observatoire de Bordeaux, Floirac </TH><TH>
Detection of OD in Selected Hot Molecular Cores </TH><TR><TH>
Baudry A.</TH><TH>
Observatoire de Bordeaux, Floirac </TH><TH>
OH Spectroscopy of the Dense Gas Surrounding Compact HII Regions </TH><TR><TH>
Bechtold J.</TH><TH>
Steward Observatory, University of Arizona </TH><TH>
Probing Dust in Quasars Observations of the 9.7 Micron Silicate Feature</TH><TR><TH>
Beckwith S.</TH><TH>
Max-Planck-Institut fuer Astronomie - Heidelberg </TH><TH>
Physical Properties of Circumstellar Disks Spectral Energy Distributions of
Young Stellar Objects</TH><TR><TH>
Beckwith S.</TH><TH>
Max-Planck-Institut fuer Astronomie - Heidelberg </TH><TH>
Search for Dust Debris in the Outer Solar System </TH><TR><TH>
Beichman C.</TH><TH>
IPAC - Pasadena </TH><TH>
Search for Dark Matter Halos in Galaxies and Clusters. </TH><TR><TH>
Bell J.</TH><TH>
NASA Ames Research Center - Moffett Field </TH><TH>
Infrared Imaging Spectroscopy of Mars </TH><TR><TH>
Bell J.</TH><TH>
NASA Ames Research Center - Moffett Field </TH><TH>
Infrared Spectroscopy of Phobos and Deimos </TH><TR><TH>
Bell Burnell J.</TH><TH>
Open University, Milton Keynes </TH><TH>
ISO Observations of Cygnus X-3 : Infrared Studies of a `Microquasar'</TH><TR><TH>
Bergeat J.</TH><TH>
Observatoire de Lyon - Saint-Genis-Laval </TH><TH>
The Environment of Cool Giant Variables
Extensions and Detached Shells On the AGB </TH><TR><TH>
Bergeron J.</TH><TH>
Institut d'Astrophysique de Paris </TH><TH>
Far IR Photometry an Spectrometry of Sub Classes of Radio-Quiet Quasars</TH><TR><TH>
Bergvall N.</TH><TH>
Uppsala Astronomical Observatory </TH><TH>
Star Formation in Luminous Blue Compact Galaxies </TH><TR><TH>
Bernard J.</TH><TH>
IAS, Orsay </TH><TH>
Of Color Variations in the ISM </TH><TR><TH>
Bezard B.</TH><TH>
Observatoire de Paris, Section de Meudon </TH><TH>
Measurement of the CH4 Mixing Ratio in Neptune's Stratosphere </TH><TR><TH>
Bezard B.</TH><TH>
Observatoire de Paris, Section de Meudon </TH><TH>
Search for Undetected Hydrocarbons On Jupiter and Saturn </TH><TR><TH>
Bezard B.</TH><TH>
Observatoire de Paris, Section de Meudon </TH><TH>
Search for Undetected Hydrocarbons On Neptune </TH><TR><TH>
Birkinshaw M.</TH><TH>
Smithsonian Institution Astrophysical Observatory </TH><TH>
IR Properties of the Cores of Nearby Radio Galaxies </TH><TR><TH>
Black J.</TH><TH>
Steward Observatory, University of Arizona </TH><TH>
Thermal Structure of Translucent Molecular Clouds </TH><TR><TH>
Blanco A.</TH><TH>
Dipartimento Di Fisica, Universita Di Lecce </TH><TH>
Dust Composition in Carbon Stars </TH><TR><TH>
Blommaert J.</TH><TH>
Institut d'Astrophysique de Paris </TH><TH>
The Nature of OH/IR Stars in the Galactic Centre </TH><TR><TH>
Blomme R.</TH><TH>
Royal Observatory of Belgium - Brussel </TH><TH>
Clumping in the Stellar Wind of Early-Type Stars </TH><TR><TH>
Bockelee-Morvan D.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Search for CO and CO2 Ices Towards Vega-Like Stars </TH><TR><TH>
Bockelee-Morvan D.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Study of Carbonaceous Matter in Comets. </TH><TR><TH>
Boisson C.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Testing the Unifying Scheme of Active Galactic Nuclei </TH><TR><TH>
Bonnet-Bidaud J.</TH><TH>
Service d'Astrophysique Saclay </TH><TH>
Infrared Study of the Peculiar X-Ray Binary Cygnus X-3 </TH><TR><TH>
Bonoli C.</TH><TH>
Osservatorio Astronomico, Padova </TH><TH>
Infrared Properties of Barred Galaxies </TH><TR><TH>
Bonoli C.</TH><TH>
Osservatorio Astronomico, Padova </TH><TH>
Infrared Properties of Galaxies in Intermediate Redshift Clusters </TH><TR><TH>
Bonoli C.</TH><TH>
Osservatorio Astronomico, Padova </TH><TH>
Star Formation in Ring Galaxies. Dust Properties in Colliding Galaxies</TH><TR><TH>
Bontemps S.</TH><TH>
Service d'Astrophysique-Saclay </TH><TH>
Mid-IR Search for Embedded Outflow Shocks Around YSOs </TH><TR><TH>
Boulanger F.</TH><TH>
IAS, Campus d'Orsay </TH><TH>
A Comparison of Extinction and Emission Properties of Dust </TH><TR><TH>
Boulanger F.</TH><TH>
IAS, Campus d'Orsay </TH><TH>
Dust in the Low Density Warm Phases of the Interstellar Medium </TH><TR><TH>
Bower G.</TH><TH>
University of California, Berkeley, </TH><TH>
Magnetic Field Morphology in Spiral Galaxies </TH><TR><TH>
Brahic A.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Reflectance Variations of Planetary Satellites. </TH><TR><TH>
Braine J.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
Is There Dust in the Intercluster Medium Dust in Galaxy Clusters</TH><TR><TH>
Braine J.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
The Interstellar Medium of a Normal, Isolated, Spiral Galaxy </TH><TR><TH>
Brand P.</TH><TH>
University of Edinburgh </TH><TH>
Warm Molecular Hydrogen in the Galaxy </TH><TR><TH>
Brandt W.</TH><TH>
IOA, Cambridge University </TH><TH>
IR Line Maps and Longwave Spectra of X-Ray Bright Extragalactic HII
Region Galaxies With Superbubbles</TH><TR><TH>
Bregman J.</TH><TH>
NASA AMES Research Center, Moffett Field </TH><TH>
Are There Hidden Supernovae? </TH><TR><TH>
Bregman J.</TH><TH>
University of Michigan, Ann Arbor </TH><TH>
Dust in the X-Ray Atmospheres of Elliptical Galaxies </TH><TR><TH>
Browne I.</TH><TH>
NRAL Jodrell Bank </TH><TH>
A New Look At the Synchrotron Emission in Radio-Loud AGN. </TH><TR><TH>
Bujarrabal V.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
Atomic Gas in Protoplanetary Nebula </TH><TR><TH>
Calzetti D.</TH><TH>
Space Telescope Science Institute - Baltimore </TH><TH>
The Relationship Between Dust Absorption and Emission in Galaxies </TH><TR><TH>
Carilli C.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Infrared Imaging of the Optical Emission Line Jet and Optical and HI
Shells in Centaurus A.</TH><TR><TH>
Carilli C.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Infrared Imaging of the Radio Hot Spots in Cygnus A. </TH><TR><TH>
Casali M.</TH><TH>
Royal Observatory, Edinburgh </TH><TH>
The Decline of Outflow Activity With YSO Age - A New Approach </TH><TR><TH>
Casali M.</TH><TH>
Royal Observatory, Edinburgh </TH><TH>
The Disks of Young Stars in Dense Clusters </TH><TR><TH>
Casoli F.</TH><TH>
Observatoire de Paris </TH><TH>
Star Formation and Gas Content in Isolated Galaxies. A Reference Sample </TH><TR><TH>
Cassinelli J.</TH><TH>
University of Wisconsin, Madison </TH><TH>
The Velocity Structure of Wolf-Rayet Winds From Infrared Line and
Continuum Observations</TH><TR><TH>
Cassinelli J.</TH><TH>
Universtiy of Wisconsin, Madison </TH><TH>
IR Diagnostics of Temperature Structure in the Atmospheres of Early B Stars</TH><TR><TH>
Ceccarelli C.</TH><TH>
CNR-IFSI and Observatoire De Grenoble </TH><TH>
Major Cooling Lines in Infall Around YSOs </TH><TR><TH>
Cernicharo J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
A Search for C3, C4H2, and C6H2 in the Interstellar Medium </TH><TR><TH>
Cernicharo J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
A Study of Dust, Atomic and Molecular Emission in Cometary Globules </TH><TR><TH>
Cernicharo J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
A Study of Water Emission in Molecular Clouds:</TH><TR><TH>
</TH><TH> </TH><TH>The Extent of Water Vapor Emission in Galactic Molecular Clouds</TH><TR><TH>
Cernicharo J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
A Study of Water Emission in O-Rich Evolved Stars: </TH><TR><TH>
</TH><TH> </TH><TH>The Water Abundance and the 17O/18O Isotopic Abundance Ratio in CSE</TH><TR><TH>
Cernicharo J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
The Mid and Far Infrared Spectrum of Keystone Molecular Clouds </TH><TR><TH>
Cernicharo J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
The Molecular Content of IRC+10216 Between 2.38 and 196.7 Microns </TH><TR><TH>
Cherchneff I.</TH><TH>
Royal Observatory of Edinburgh </TH><TH>
Observation of Dust Features in Carbon-Rich Wolf-Rayet Stars </TH><TR><TH>
Cherchneff I.</TH><TH>
Royal Observatory of Edinburgh </TH><TH>
Observation of Dust Features in R CRB Stars </TH><TR><TH>
Chini R.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
ISO Study of Protostars </TH><TR><TH>
Chini R.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
Star Formation Efficiency in Galaxies </TH><TR><TH>
Chrysostomou A.</TH><TH>
University of Hertfordshire - Hatfield </TH><TH>
Determining the Role of Magnetic Fields in the Disks of YSOs </TH><TR><TH>
Chrysostomou A.</TH><TH>
University of Hertfordshire - Hatfield </TH><TH>
Line Emission From Photodissociation Regions </TH><TR><TH>
Clampin M.</TH><TH>
STSCI - Baltimore </TH><TH>
Dust Characterization in Circumstellar Shells Around Evolved, Massive Stars</TH><TR><TH>
Clark F.</TH><TH>
Phillips Laboratory, Geophysics </TH><TH>
Emission From and Destruction of Small Interstellar Dust High
Radiation Environments</TH><TR><TH>
Clavel J.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Mapping the Molecular Torus in Active Galactic Nuclei </TH><TR><TH>
Clayton G.</TH><TH>
CASA, University of Colorado - Boulder </TH><TH>
Understanding the Evolution of H-Deficient Stars </TH><TR><TH>
Clemens D.</TH><TH>
Boston University </TH><TH>
Are Starless Bok Globules Really Devoid of Stars? </TH><TR><TH>
Clemens D.</TH><TH>
Boston University </TH><TH>
Dust Temperatures and Densities in Filamentary Dark Clouds </TH><TR><TH>
Clemens D.</TH><TH>
Boston University </TH><TH>
Embedded Magnetic Fields in Filamentary Dark Clouds </TH><TR><TH>
Clemens D.</TH><TH>
Boston University </TH><TH>
Low Luminosity Protostars and YSOs in Bok Globules </TH><TR><TH>
Clements D.</TH><TH>
Oxford University - Oxford </TH><TH>
ISO Observations of Low Ionisation BAL Quasars </TH><TR><TH>
Clements D.</TH><TH>
Oxford University - Oxford </TH><TH>
The Spectral Energy Distribution of Extreme Ultraluminous IRAS Galaxies</TH><TR><TH>
Coe M.</TH><TH>
Southampton Universiy - Southampton </TH><TH>
TOO: Studies of High Mass X-Ray Binary Systems </TH><TR><TH>
Cohen M.</TH><TH>
University of California-Berkeley </TH><TH>
PAH Emission Bands in Selected Planetary Nebulae </TH><TR><TH>
Colangeli L.</TH><TH>
Osservatorio Astronomico Di Capodimonte, Napoli </TH><TH>
Cometary Nuclei and Trails Study Analysis of Comets </TH><TR><TH>
Colgan S.</TH><TH>
SETI Institute/NASA-AMES Research Center </TH><TH>
Infrared Spectroscopy of the Great Annihilator </TH><TR><TH>
Colgan S.</TH><TH>
SETI Institute/NASA-AMES Research Center </TH><TH>
The Properties of Narrow Recombination Line HII Regions </TH><TR><TH>
Combes F.</TH><TH>
DEMIRM, Observatoire De Paris </TH><TH>
Bars and Tides in Galaxies Role of Large-Scale Dynamics On Star Formation</TH><TR><TH>
Combes F.</TH><TH>
DEMIRM, Observatoire De Paris </TH><TH>
Spiral Arm in Messier 31 Star-Formation Processes Across the Arm</TH><TR><TH>
Comeron F.</TH><TH>
University of Barcelona </TH><TH>
Brown Dwarf Candidates in Embedded Stellar Populations </TH><TR><TH>
Cotera A.</TH><TH>
Stanford University - Moffett Field </TH><TH>
The Interaction of Recently Discovered Hot Stars With Galactic Centre
Thermal Radio Emission Filaments</TH><TR><TH>
Courtin R.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
A Spectroscopic Investigation of Titan At 5-7 Micrometers </TH><TR><TH>
Courvoisier T.</TH><TH>
Geneva Observatory - Sauverny </TH><TH>
ISO Spectra of a Sample of AGN</TH><TR><TH>
Courvoisier T.</TH><TH>
Geneva Observatory - Sauverny </TH><TH>
Polarimetry of 2 Radio-Loud Quasars </TH><TR><TH>
Coustenis A.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Spectroscopy of the 15 Micron Region On Titan (CO2 and CO) </TH><TR><TH>
Coustenis A.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Spectroscopy of the 16 Micron Region on Titan (C4H2 and C3H4) </TH><TR><TH>
Cox C.</TH><TH>
University of Michigan - Ann Arbor </TH><TH>
Far Infrared Emission From the Cores of Rich Clusters </TH><TR><TH>
Cox P.</TH><TH>
Observatoire de Marseille </TH><TH>
Spectroscopic Observations of PDRs in Proto-Planetary and Planetary Nebulae</TH><TR><TH>
Cox P.</TH><TH>
Observatoire de Marseille </TH><TH>
The Helix Planetary Nebula: A Case Study of a PDR Region</TH><TR><TH>
Creech-Eakman M.</TH><TH>
University of Denver, Dept. of Physics and Astronomy </TH><TH>
Stellar Plasma to Circumstellar Dust Transformation </TH><TR><TH>
Crifo F.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Bolometric Magnitude and Effective Temperature of M Dwarfs</TH><TR><TH>
Crifo F.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Radii, Effective Temperatures and Bolometric Luminosities of Subdwarfs</TH><TR><TH>
Crotts A.</TH><TH>
Columbia University - New York </TH><TH>
Evolution of 3-35 Micron Lines From the Formation of SNR 1987a </TH><TR><TH>
Crovisier J.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
TOO: Observations of Unexpected Comets. </TH><TR><TH>
Cruikshank D.</TH><TH>
NASA AMES Research Center - Moffett Field </TH><TH>
Molecular Nitrogen in Interstellar Ices </TH><TR><TH>
Currie D.</TH><TH>
University of Maryland - College Park </TH><TH>
Thermal Structure and History of Eta Car </TH><TR><TH>
Danziger J.</TH><TH>
ESO - Garching </TH><TH>
TOO: Supernovae Mid-IR Supernova Studies</TH><TR><TH>
Davies J.</TH><TH>
University of Wales - Cardiff </TH><TH>
The Diffuse FIR Emission From Spiral Galaxies </TH><TR><TH>
De Jong R.</TH><TH>
Kapteyn Astronomical Institute - Groningen </TH><TH>
Surface Density Distribution of Hot and Cold Dust in a Complete Sample
Of Face-On Spiral Galaxies. </TH><TR><TH>
De Zotti G.</TH><TH>
Osservatorio Astronomico, Padova </TH><TH>
Far-IR Evolution of Galaxies: The IRAS Deep Survey Sample. </TH><TR><TH>
Decourchelle A.</TH><TH>
Service d'Astrophysique, Ce Saclay </TH><TH>
Detailed Comparison of IR and X-Ray Emission in Selected Regions of
The Cygnus Loop Supernova Remnant.</TH><TR><TH>
Deguchi S.</TH><TH>
National Astronomical Observatory - Nagano </TH><TH>
Observations of H2O Thermal Lines in Nuclei of Galaxies </TH><TR><TH>
Deguchi S.</TH><TH>
National Astronomical Observatory - Nagano </TH><TH>
Observations of Halo AGB Stars With ISO SWS </TH><TR><TH>
Deguchi S.</TH><TH>
National Astronomical Observatory - Nagano </TH><TH>
Observations of Stars With Unusual IRAS LRS Spectra </TH><TR><TH>
Deleuil M.</TH><TH>
Laboratoire d'Astronomie Spatiale - Marseille </TH><TH>
Origin of the Circumstellar Gas Around Beta Pictoris </TH><TR><TH>
Dennefeld M.</TH><TH>
Institut d'Astrophysique de Paris </TH><TH>
The Nature of High X-Luminosity Rosat/IRAS Galaxies: </TH><TR><TH>
</TH><TH> </TH><TH>Relations With Narrow-Line Seyfert 1 Galaxies</TH><TR><TH>
Dennefeld M.</TH><TH>
Institut d'Astrophysique de Paris </TH><TH>
The Nature of the Faintest IRAS Galaxies and Galaxy Evolution </TH><TR><TH>
Dermott S.</TH><TH>
Univ of Florida, Gainesville </TH><TH>
Observations of the Earth's Circumsolar Dust Ring </TH><TR><TH>
d'Hendecourt L.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay </TH><TH>
Far Infrared Spectroscopy of Ices Features </TH><TR><TH>
d'Hendecourt L.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay </TH><TH>
Search for Specific Solid State Features From Interstellar Grains </TH><TR><TH>
Di Serego Alighieri </TH><TH>
Osservatorio Astrofisico di Arcetri - Firenze </TH><TH>
Jet-ISM Interactions in Radio Galaxies. </TH><TR><TH>
Digel S.</TH><TH>
Harvard-Smithsonian Center for Astrophysics </TH><TH>
Abundance Determinations in the Far Outer Galaxy </TH><TR><TH>
Dobashi K.</TH><TH>
Materials Science,University of Osaka Prefecture, Sakai </TH><TH>
Infrared Properties of YSO Candidates Isolated From Molecular Clouds </TH><TR><TH>
Doi Y.</TH><TH>
The Institute for Space and Astronautical Science, Kanagawa </TH><TH>
Spectroscopy of Interstellar Gas Around the Cygnus OB2 Association </TH><TR><TH>
Donahue M.</TH><TH>
Space Telescope Science Institute </TH><TH>
ISO Studies of Cooling-Flow Emission-Line Nebulae </TH><TR><TH>
Dougados C.</TH><TH>
Laboratoire d'Astrophysique de Grenoble </TH><TH>
The Embedded Clusters Associated With Young Intermediate Mass Stars</TH><TR><TH>
Doyle J.</TH><TH>
Armagh Observatory - Armagh </TH><TH>
Detectability of Mass Loss From Cool M Dwarfs </TH><TR><TH>
Drapatz S.</TH><TH>
MPIE, Garching </TH><TH>
Search for Interstellar Molecular Oxygen </TH><TR><TH>
Drossart P.</TH><TH>
DESPA, Observatoire de Meudon </TH><TH>
Spectroscopy of the Auroral Regions of Jupiter </TH><TR><TH>
Dufton P.</TH><TH>
Queen's University Belfast - Belfast </TH><TH>
H II Regions Associated With Young Galactic Clusters </TH><TR><TH>
Dunlop J.</TH><TH>
Liverpool John Moores University - Liverpool </TH><TH>
The Formation and Evolution of Elliptical Galaxies </TH><TR><TH>
Dutrey A.</TH><TH>
IRAM, Saint-Martin-d'Heres </TH><TH>
Chemistry of CO in Circumstellar Disks Around YSO's </TH><TR><TH>
Dwek E.</TH><TH>
Nasa Goddard Space Flight Center, Greenbelt </TH><TH>
Grain Destruction in Supernova Remnants </TH><TR><TH>
Eaton J.</TH><TH>
Tennessee State University - Nashville </TH><TH>
The Atmospheric Eclipse of V444 Cygni </TH><TR><TH>
Eckart A.</TH><TH>
MPE - Garching </TH><TH>
Probing Shocks and PDRs Using Sulphur-Bearing Molecules </TH><TR><TH>
Edmunds M.</TH><TH>
Physics and Astronomy, Cardiff University </TH><TH>
The Cooling and Composition of Extragalactic HII Regions </TH><TR><TH>
Egami E.</TH><TH>
Institute for Astronomy, Univ. of Hawaii </TH><TH>
Search for Primeval Galaxies Around Z>4 Quasars </TH><TR><TH>
Ehrenfreund P.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Far-Infrared Observations of Water Ice </TH><TR><TH>
Ehrenfreund P.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Search for Solid O2 and O3 On Interstellar Grains With ISO </TH><TR><TH>
Eisloeffel J.</TH><TH>
Observatoire de Grenoble - Grenoble Cedex </TH><TH>
Rotationally-Excited Molecular Hydrogen in Bipolar Outflows </TH><TR><TH>
Elbaz D.</TH><TH>
CEA,DSM,DAPNIA, Service d'Astrophysique </TH><TH>
Galaxy Evolution and Diffuse FIR Emission in Hickson Compact Groups of
Galaxies</TH><TR><TH>
Elias J.</TH><TH>
Cerro Tololo Inter-American Observatory, NOAO </TH><TH>
Comparison of Mass-Losing AGB Stars in the Magellanic Clouds</TH><TR><TH>
Elston R.</TH><TH>
National Optical Astronomy Observatories, Tucson </TH><TH>
The Nature of Faint Red Field Galaxies </TH><TR><TH>
Emery R.</TH><TH>
Rutherford Appleton Laboratory - Didcot </TH><TH>
Study of the Rosette Nebula Complex </TH><TR><TH>
Encrenaz T.</TH><TH>
Paris Observatory - Meudon </TH><TH>
Neptune: Search for PH3 and Determination of Tropospheric C/H </TH><TR><TH>
Engelmann J.</TH><TH>
Sternwarte Der Universitaet Bonn </TH><TH>
Interaction of IVC 86+38-44 With the Hot Plasma </TH><TR><TH>
Engels D.</TH><TH>
Hamburger Sternwarte - Hamburg </TH><TH>
IR Spectral Properties of Young PPN </TH><TR><TH>
Engels D.</TH><TH>
Hamburger Sternwarte - Hamburg </TH><TH>
The 22 Ghz H2O Maser Pump in AGB Stars </TH><TR><TH>
Eriksson K.</TH><TH>
Uppsala astronomical observatory</TH><TH>
Imaging of Dust Shells Around Carbon Stars </TH><TR><TH>
Eriksson K.</TH><TH>
Uppsala astronomical observatory</TH><TH>
Spectra of Envelopes Around AGB Stars </TH><TR><TH>
Evans A.</TH><TH>
Keele University, Staffordshire </TH><TH>
An ISO Study of PAH Emission in XX Oph </TH><TR><TH>
Evans A.</TH><TH>
Keele University, Staffordshire </TH><TH>
Far Infrared Observations of RV Tauri Stars </TH><TR><TH>
Evans A.</TH><TH>
Keele University, Staffordshire </TH><TH>
The Far-Infrared Flux Distribution of Rs Cvn Stars </TH><TR><TH>
Evans N.</TH><TH>
The Uni. of Texas at Austin, TX </TH><TH>
Photoionization Regulated Star Formation, Cloud Structure, and Tracers
Of the Neutral ISM</TH><TR><TH>
Fabian A.</TH><TH>
Institute of Astronomy, Cambridge </TH><TH>
Cold Gas and Star Formation in Massive Cooling Flows </TH><TR><TH>
Falcke H.</TH><TH>
Max-Planck-Institut fuer Radioastronomie - Bonn </TH><TH>
Photometry of a New Sample of Ghz--Peaked--Spectrum Sources </TH><TR><TH>
Falgarone E.</TH><TH>
Ecole Normale Superieure - Paris </TH><TH>
Gas Spectral Diagnostics of the Dust Emission, Color Variations in
Interstellar Clouds.</TH><TR><TH>
Fanti C.</TH><TH>
Insititute of Radioastronomy Bologna </TH><TH>
Medium-Far Infrared Observations of Compact Steep-Spectrum and Ghz
Peaked Spectrum Radio Galaxies</TH><TR><TH>
Fender R.</TH><TH>
Open University, Milton Keynes </TH><TH>
TOO: ISO Observations of Cygnus X-3 in Outburst </TH><TR><TH>
Feretti L.</TH><TH>
Istituto Di Radioastronomia - Bologna </TH><TH>
Rich Clusters With Tailed Radio Galaxies: Dust and Stripping </TH><TR><TH>
Ferrari C.</TH><TH>
EUROPA, Paris Observatory - Meudon </TH><TH>
Reflectance Variations in Saturn'S Rings. Rings Spectrum</TH><TR><TH>
Festou M.</TH><TH>
Observatoire Midi-Pyrenees - Toulouse </TH><TH>
Production and Loss of H3O+ Ions in Comet Comae. Water Ions</TH><TR><TH>
Fitzsimmons A.</TH><TH>
Queens University of Belfast - Belfast </TH><TH>
The Composition of D-Type Asteroids </TH><TR><TH>
Fix J.</TH><TH>
University of Iowa - Iowa City </TH><TH>
ISO Observations of Variable Circumstellar Shells </TH><TR><TH>
Forrest W.</TH><TH>
University of Rochester - Rochester, NY </TH><TH>
A Search for Brown Dwarfs in the Hyades </TH><TR><TH>
Fosbury R.</TH><TH>
ST\ ECF Garching </TH><TH>
Infrared Properties of Extragalactic Radio Sources </TH><TR><TH>
Foster R.</TH><TH>
Naval Research Laboratory - Washington, DC </TH><TH>
Circumstellar Dust Emission From Millisecond Pulsars </TH><TR><TH>
Franceschini A.</TH><TH>
Osservatorio Astronomico di Padova </TH><TH>
ISO Observations of Candidate Primeval Dusty Galaxies </TH><TR><TH>
Fuente A.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
A Chemical Study of the Hot and Dense Molecular Gas Adjacent to
Photodissociation Regions </TH><TR><TH>
Fuente A.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
Study of the Interface Between the Atomic and Molecular Gas in the
Reflection Nebulae: NGC 2068 (S), Sgr R1 (A)</TH><TR><TH>
Furniss I.</TH><TH>
Dept of Physics and Astronomy UCL - London </TH><TH>
Observations of Complex HII/Molecular Cloud Structures </TH><TR><TH>
Fusi Pecci F.</TH><TH>
Osservatorio Astronomico, Bologna </TH><TH>
Circumstellar Matter in the Central Region of Globular Clusters. </TH><TR><TH>
Gallant Y.</TH><TH>
MPIK, Heidelberg</TH><TH>
Crab-Like Supernova Remnants Imaging, Polarisation and Broad-Band Spectroscopy</TH><TR><TH>
Garcia-Lario P.</TH><TH>
ESA IUE Observatory - Madrid </TH><TH>
Correlation of Mass and Age With the Far-IR Colors of Pne and Ppne </TH><TR><TH>
Garcia-Vargas M.</TH><TH>
Dpto Fisica Teorica. Univ. Autonoma De Madrid. </TH><TH>
IR Study of High Metallicity Star-Forming Regions </TH><TR><TH>
Garnett D.</TH><TH>
University of Minnesota, Minneapolis </TH><TH>
Sulfur and Neon in Extragalactic HII Regions </TH><TR><TH>
Garzon F.</TH><TH>
Instituto De Astrofisica De Canarias - La Laguna </TH><TH>
Stellar Populations of the Inner Bulge of the Galaxy. </TH><TR><TH>
Gavazzi G.</TH><TH>
Osservatorio Astronomico Di Brera - Milano </TH><TH>
IR Properties of S/Irr Galaxies in the Coma and A1367 Clusters </TH><TR><TH>
Gehrz R.</TH><TH>
University of Minnesota, Minneapolis </TH><TH>
Studies of Classical Novae and Related Objects With ISO </TH><TR><TH>
Gehrz R.</TH><TH>
University of Minnesota, Minneapolis </TH><TH>
TOO: Observations of New Novae in Outburst </TH><TR><TH>
Genzel R.</TH><TH>
MPIE, Garching </TH><TH>
Testing Unified Models With Infrared Spectroscopy </TH><TR><TH>
Gerbaldi M.</TH><TH>
Institut d'Astrophysique Paris </TH><TH>
Remnant of Circumstellar Matter Around Early A-Type Stars in Young Clusters</TH><TR><TH>
Gerin M.</TH><TH>
Radioastronomie, Ecole Normale Superieure, Paris </TH><TH>
The Dust Composition At High Redshift </TH><TR><TH>
Giard M.</TH><TH>
CESR/CNRS - Toulouse </TH><TH>
Warm Dust in HII Regions and PDRs </TH><TR><TH>
Giard M.</TH><TH>
CESR/CNRS - Toulouse </TH><TH>
Water Vapor in Warm Dusty Regions </TH><TR><TH>
Gilmore G.</TH><TH>
Institute of Astronomy - Cambridge </TH><TH>
Brown Dwarf Halos of Low Redshift Spiral Galaxies </TH><TR><TH>
Goebel J.</TH><TH>
NASA Ames Research Center, Moffett Field </TH><TH>
Study of the Population Distribution of the 7
micron dust emission feature in oxygen-rich stars </TH><TR><TH>
Goldschmidt P.</TH><TH>
Imperial College, London </TH><TH>
The Physical Causes of Quasar Evolution </TH><TR><TH>
Gonzalez-Serrano J.</TH><TH>
Universidad De Cantabria - Santander </TH><TH>
IR Photometry of a Complete Sample of B2 Radio Quasars </TH><TR><TH>
Goodman A.</TH><TH>
Harvard University Astronomy Department </TH><TH>
Mapping Magnetic Fields in the Interstellar Medium </TH><TR><TH>
Gorny S.</TH><TH>
Nicolaus Copernicus Astronomical Center - Torun </TH><TH>
Spectroscopy of Dusty Planetary Nebulae With Wr-Type Central Stars </TH><TR><TH>
Grady C.</TH><TH>
Applied Research Corporation - Landover </TH><TH>
The Beta Pictoris Phenomenon in Young Stars With Accreting Gas</TH><TR><TH>
Gray M.</TH><TH>
University of Bristol - Bristol </TH><TH>
Detection of OH FIR Lasers in Star-Forming Regions </TH><TR><TH>
Green D.</TH><TH>
Mullard Radio Astronomy Observatory - Cambridge </TH><TH>
Mapping of 3C58 </TH><TR><TH>
Greenhouse M.</TH><TH>
Smithsonian Institution - Washington DC </TH><TH>
Infrared Coronal Lines of Active Galactic Nuclei </TH><TR><TH>
Gregorini L.</TH><TH>
IRA - CNR - Bologna </TH><TH>
A Complete Sample of Dumb-Bell Galaxies Dust Inside Interacting Systems</TH><TR><TH>
Griffin M.</TH><TH>
Queen Mary and Westfield College, London </TH><TH>
The Far Infrared Continuum Spectra of Cold Protostellar Sources </TH><TR><TH>
Groenewegen M.</TH><TH>
Institut d'Astrophysique De Paris </TH><TH>
Observations of Mass Losing Supergiants in the Magellanic Clouds </TH><TR><TH>
Grossmann V.</TH><TH>
Astronomisches Institut Der Universitaet Tuebingen </TH><TH>
Cold Dust and Dust Filaments in a High-Latitude Cirrus Cloud </TH><TR><TH>
Gruen E.</TH><TH>
MPIK, Heidelberg </TH><TH>
TOO: ISOPHOT Observations of a Bright Comet </TH><TR><TH>
Guelin M.</TH><TH>
IRAM, Saint Martin d'Heres </TH><TH>
FIR Emission in the Cepheus A/B Molecular Complex </TH><TR><TH>
Guelin M.</TH><TH>
IRAM, Saint Martin d'Heres </TH><TH>
Matter At the Periphery of Nearby Galaxies: the Dust Component </TH><TR><TH>
Guenther E.</TH><TH>
Queen Mary and Westfield College, London </TH><TH>
Ex-Orionis Stars </TH><TR><TH>
Guertler J.</TH><TH>
Universitaets-Sternwarte - Jena </TH><TH>
Analysis of Dust Envelopes Around Evolved Stars </TH><TR><TH>
Guesten R.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
Low-Mass Protostars in Globular Filament GF-9 </TH><TR><TH>
Guesten R.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
Study of An Unusual Shock Region in the Galactic Center. </TH><TR><TH>
Haas M.</TH><TH>
NASA-AMES Research Center - Moffett Field </TH><TH>
Physical Conditions in the Circumstellar Envelopes of Supergiants </TH><TR><TH>
</TH><TH> </TH><TH>And Other Evolved Stars</TH><TR><TH>
Haikala L.</TH><TH>
Helsinki University Observatory - Helsinki </TH><TH>
Mapping of Cold Dust and Search for Embedded Young Stars </TH><TR><TH>
Hammer F.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Infrared Studies of Distant Galaxies in Deep Optical Radio Surveys. </TH><TR><TH>
Hammersley P.</TH><TH>
Instituto De Astrofisica De Canarias - La Laguna </TH><TH>
Star Counts in the Galactic Bar. </TH><TR><TH>
Hansen L.</TH><TH>
Copenhagen University Observatory - Copenhagen </TH><TH>
Production and Destruction of Dust in X-Ray Gas Environments</TH><TR><TH>
Harrington P.</TH><TH>
University of Maryland - College Park, Maryland </TH><TH>
Dust in Hydrogen-Poor Planetary Nebulae </TH><TR><TH>
Harris A.</TH><TH>
DLR Institute for Planetary Exploration, Berlin </TH><TH>
Cometary Activity in Asteroids </TH><TR><TH>
Harvey P.</TH><TH>
University of Texas at Austin - Austin, Texas </TH><TH>
Diffraction Limited Imaging of Protostellar Clouds </TH><TR><TH>
Hauschildt P.</TH><TH>
Arizona State University - Tempe </TH><TH>
A Spectroscopic Study of the Water Bands in M Dwarfs </TH><TR><TH>
Hawley S.</TH><TH>
Michigan State University - East Lansing </TH><TH>
Circumstellar Disks and Far Ir Luminosity in Active M Dwarfs </TH><TR><TH>
Heithausen A.</TH><TH>
I. Physikalisches Institut Der Universitaet Zu Koeln </TH><TH>
Ionized Carbon in High Velocity Clouds </TH><TR><TH>
Helmich F.</TH><TH>
Sterrewacht Leiden - Leiden </TH><TH>
Searches for New Interstellar Molecules: CH2 and NCCN </TH><TR><TH>
Helou G.</TH><TH>
IPAC - Pasadena </TH><TH>
Exceptions to the Radio-Infrared Correlation: Radio-Deficient Galaxies</TH><TR><TH>
Henkel C.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
An OH Multilevel Study of Megamaser Galaxies OH Megamasers</TH><TR><TH>
Henkel C.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
The Strongest Molecular Hotspot in the Magellanic Clouds </TH><TR><TH>
Henning P.</TH><TH>
University of New Mexico - Albuquerque </TH><TH>
Dust in the Intergalactic Hi Cloud Near UGC7636 </TH><TR><TH>
Henning T.</TH><TH>
Max Planck Group - Jena </TH><TH>
Dust Spectroscopy of Embedded Infrared Sources in the Magellanic Clouds</TH><TR><TH>
Herbstmeier U.</TH><TH>
Max-Planck-Institut Fuer Astronomie - Heidelberg </TH><TH>
Physical Properties of a Cloud Located in the Local Hot Bubble </TH><TR><TH>
Higdon J.</TH><TH>
NRAO - Socorro </TH><TH>
Probing the Star Forming ISM in Ring Galaxies</TH><TR><TH>
Hines D.</TH><TH>
Steward Observatory - Tucson </TH><TH>
Infrared Fine Structure Emission in Warm IR-Ultraluminous AGN </TH><TR><TH>
Hirth G.</TH><TH>
Max Planck Institut Fuer Astronomie - Heidelberg </TH><TH>
Physical Properties of Outflows From Young Stellar Objects </TH><TR><TH>
Hoare M.</TH><TH>
Max-Planck-Institut fuer Astronomie - Heidelberg </TH><TH>
Ionized Winds From Luminous Young Stellar Objects. </TH><TR><TH>
Hoernes P.</TH><TH>
Max-Planck-Institut Fuer Radioastronomie - Bonn </TH><TH>
Dust, Clouds and Magnetic Fields in a SW Spiral Arm Region of M31 </TH><TR><TH>
Hora J.</TH><TH>
Institute for Astronomy, University of Hawaii </TH><TH>
The Spatial Distribution of Cool Dust in Planetary Nebulae </TH><TR><TH>
Hough J.</TH><TH>
University of Hertfordshire - Hatfield </TH><TH>
Polarimetry of the Nuclear Regions of Cena </TH><TR><TH>
Hough J.</TH><TH>
University of Hertfordshire - Hatfield </TH><TH>
Polarimetry of the Nucleus of Active Galaxies </TH><TR><TH>
Hrivnak B.</TH><TH>
Valparaiso University, Indiana </TH><TH>
SWS Spectroscopy of Obscured Proto-Planetary Nebulae </TH><TR><TH>
Hrivnak B.</TH><TH>
Varparaiso University, Indiana </TH><TH>
Spectroscopy of Visible Proto-Planetary Nebulae </TH><TR><TH>
Hron J.</TH><TH>
Institut fuer Astronomie, Universitaet Wien - Vienna </TH><TH>
Spectral Variability of Long Period Variables </TH><TR><TH>
Hu E.</TH><TH>
Institute for Astronomy - Honolulu </TH><TH>
Two Extremely Red Galaxies </TH><TR><TH>
Huettemeister S.</TH><TH>
Harvard-Smithsonian Center for Astrophysics </TH><TH>
Dust Properties of Galactic Center Clouds </TH><TR><TH>
Hurley K.</TH><TH>
University of California At Berkeley </TH><TH>
Study of Soft Gamma Repeater Counterparts </TH><TR><TH>
Hurt R.</TH><TH>
UC Riverside Dept. of Physics - Riverside, CA </TH><TH>
Dust Emission From Class 0 Protostars in the Serpens Cloud Core </TH><TR><TH>
Hutsemekers D.</TH><TH>
Liege Institute of Astrophysics - Liege </TH><TH>
Dust Around Luminous Early-Type Stars in Nearby Galaxies </TH><TR><TH>
Hutsemekers D.</TH><TH>
Liege Institute of Astrophysics - Liege </TH><TH>
The Circumstellar Environment of HD168625 </TH><TR><TH>
Iovino A.</TH><TH>
Osservatorio Astronomico Di Brera, Milano </TH><TH>
ISO Observations of Compact Groups of Galaxies. </TH><TR><TH>
Ip W.</TH><TH>
Max-Planck-Institut Fuer Aeronomie, Lindau </TH><TH>
A Survey of Kuiper Belt Candidates </TH><TR><TH>
Ivison R.</TH><TH>
Royal Observatory, Edinburgh </TH><TH>
Testing the Binary Hypothesis for OH/IR Colour Mimics </TH><TR><TH>
Ivison R.</TH><TH>
Royal Observatory, Edinburgh </TH><TH>
The Properties of Circumstellar Dust in Symbiotic Miras </TH><TR><TH>
Jackson J.</TH><TH>
Boston University, MA </TH><TH>
Photodissociated Gas in the NGC 6334 Complex </TH><TR><TH>
Jaffe D.</TH><TH>
University of Texas at Austin, TX </TH><TH>
Low Velocity Shocks in the Dense Interstellar Medium </TH><TR><TH>
Jaffe W.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Cool Gas and Dust in Cooling Flows in Clusters of Galaxies </TH><TR><TH>
Jameson R.</TH><TH>
Leicester University - Leicester </TH><TH>
A Spectral Atlas for M Dwarfs </TH><TR><TH>
Jansen D.</TH><TH>
Sterrewacht Leiden - Leiden </TH><TH>
The O/OH/H2O Transition in Partially Ionized Globules in IC1396 </TH><TR><TH>
Jarrett T.</TH><TH>
IPAC - Pasadena </TH><TH>
Multi-Wavelength Study of Starburst NGC 3690 </TH><TR><TH>
Jenniskens P.</TH><TH>
NASA/AMES Research Center - Moffett Field </TH><TH>
The Emission Spectrum of Quiescent Dense Cloud Dust. </TH><TR><TH>
Jiang B.</TH><TH>
National Astronomical Observatory - Nagano </TH><TH>
The Nature of IRAS LRS Sources Without Near-Infrared Detection </TH><TR><TH>
Joblin C.</TH><TH>
NASA AMES Research Center - Moffett Field </TH><TH>
Photochemical Evolution of PAHs in the Interstellar Medium</TH><TR><TH>
Jones H.</TH><TH>
Institute for Astronomy - Edinburgh </TH><TH>
Water Vapour in Cool Dwarfs </TH><TR><TH>
Jorissen A.</TH><TH>
Institut d'Astronomie d'Astrophysique, Bruxelles </TH><TH>
A Study of Mass Loss Along the AGB and RGB of 47 Tuc </TH><TR><TH>
Jorissen A.</TH><TH>
Institut d'Astronomie d'Astrophysique, Bruxelles </TH><TH>
Dust in Binaries Containing Chemically Peculiar Giants </TH><TR><TH>
Jorissen A.</TH><TH>
Institut d'Astronomie d'Astrophysique, Bruxelles </TH><TH>
IR Spectral Classification of S Stars </TH><TR><TH>
Jourdain De Muizon M.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
The Organic Component of Interstellar Dust in Diffuse Clouds </TH><TR><TH>
Kaper L.</TH><TH>
European Southern Observatory - Garching </TH><TH>
Infrared Study of Low-Mass X-Ray Binaries </TH><TR><TH>
Kaper L.</TH><TH>
European Southern Observatory - Garching </TH><TH>
Stellar-Wind Structure in High-Mass X-Ray Binaries </TH><TR><TH>
Kastner J.</TH><TH>
Massachusetts Institute of Technology, Cambridge </TH><TH>
Mid-IR Polarimetric Imaging of Evolved Star Envelopes </TH><TR><TH>
Kawara K.</TH><TH>
Dept. of Astron. Sci., Mitaka, Tokyo </TH><TH>
A Search for Primeval Galaxies Around Known Objects</TH><TR><TH>
Kawara K. </TH><TH>
Dept. of Astron. Sci., Mitaka, Tokyo </TH><TH>
MIR and FIR Photometry of High-Redshift Qsos </TH><TR><TH>
Keel W.</TH><TH>
University of Alabama - Tuscaloosa </TH><TH>
Dust Emission and Absorption in Backlit Spiral Galaxies </TH><TR><TH>
Keenan F.</TH><TH>
Queen's University Belfast </TH><TH>
Spectroscopy of Hot Halo PAGB Stars and Planetary Nebulae </TH><TR><TH>
Kegel W.</TH><TH>
Inst. f. Theor. Physik, Universitaet Frankfurt/Main </TH><TH>
Methanol-Masers: Pump Mechanism and Possible Iraser-Lines </TH><TR><TH>
Kegel W.</TH><TH>
Inst. f. Theor. Physik, Universitaet Frankfurt/Main </TH><TH>
Oh-Megamasers: Pump Mechanism, Possible Iraser-Lines, and the Velocity Field.</TH><TR><TH>
Kerp J.</TH><TH>
Radioastronomisches Institut der Universitaet Bonn </TH><TH>
The High-Velocity-Cloud 90+42.5-130 </TH><TR><TH>
Kerschbaum F.</TH><TH>
Institut fuer Astronomie, Universitaet Wien - Vienna </TH><TH>
Atmospheric Structure of Oxygen-Rich Semiregular Variables </TH><TR><TH>
Kidger M.</TH><TH>
Instituto De Astrofisica De Canarias - La Laguna </TH><TH>
The Optical-Radio Polarisation Breakpoint in Blazars </TH><TR><TH>
Knapp G.</TH><TH>
Princeton University Observatory - Princeton </TH><TH>
Origin and Evolution of Dust in Elliptical Galaxies </TH><TR><TH>
Koch-Miramond L.</TH><TH>
CEA/DAPNIA/Astrophysique - Gif-sur-Yvette </TH><TH>
Search for Circumstellar Material Around Nearby Pulsars </TH><TR><TH>
Koester B.</TH><TH>
I. Physikalisches Institut, Universitaet Zu Koeln </TH><TH>
CO Emission From Massive Star Formation Regions </TH><TR><TH>
Koornneef J.</TH><TH>
SRON-G - Groningen </TH><TH>
An Investigation of the Ara Infrared Cluster </TH><TR><TH>
Koornneef J.</TH><TH>
SRON-G - Groningen </TH><TH>
Search for Cold Molecular Hydrogen in the Galaxy </TH><TR><TH>
Krishna G.</TH><TH>
Max-Planck-Institut fuer Radioastronomie - Bonn </TH><TH>
Mid and Far-Infrared Properties of Nearby Radio-Loud Ellipticals </TH><TR><TH>
Krueger H.</TH><TH>
Max-Planck-Institut Fuer Astronomie - Heidelberg </TH><TH>
Infrared Studies of HII Galaxies with Companions </TH><TR><TH>
Krugel E.</TH><TH>
Max-Planck-Institut fur Radioastronomie - Bonn </TH><TH>
Dust Emission from Radio Galaxies at High Redshifts </TH><TR><TH>
Kunth D.</TH><TH>
Institut d'Astrophysique De Paris </TH><TH>
PAH Molecules in Star-Forming Galaxies </TH><TR><TH>
Kutner M.</TH><TH>
Rensselaer Polytechnic Institute - Troy </TH><TH>
Molecular Clouds and Star Forming Regions in the Magellanic Clouds </TH><TR><TH>
Kwok S.</TH><TH>
University of Calgary, Alberta </TH><TH>
Spectroscopy of 21 Micron Feature Sources </TH><TR><TH>
Kwok S.</TH><TH>
University of Calgary, Alberta </TH><TH>
Spectroscopy of Extreme Carbon Stars </TH><TR><TH>
Lada E.</TH><TH>
University of Maryland, College Park, Maryland </TH><TH>
Investigations of the Earliest Stages of Stellar Evolution in Young
Embedded Clusters</TH><TR><TH>
Lagage P.</TH><TH>
CEA, DSM/DAPNIA/Service d'Astrophysique, Saclay </TH><TH>
Polarimetry of Dust Disks Around MS and PMS Stars. </TH><TR><TH>
Lagrange A.</TH><TH>
Observatoire De Grenoble - Grenoble </TH><TH>
Infra-Red Study of the Close HAEBE Binary System TY CrA </TH><TR><TH>
Lahuis F.</TH><TH>
Rutherford Appleton Laboratory Didcot </TH><TH>
HII Regions in M33, Supernovae Rates</TH><TR><TH>
Lambert D.</TH><TH>
Univ of Texas at Austin </TH><TH>
FG Sagittae--A New R Corona Borealis Star </TH><TR><TH>
Lambert D.</TH><TH>
Univ of Texas at Austin </TH><TH>
Infrared Spectroscopy of R Coronae Borealis Stars </TH><TR><TH>
Lambert D.</TH><TH>
Univ of Texas at Austin </TH><TH>
Testing Model Atmospheres of Cool Dwarf Stars With ISO </TH><TR><TH>
Lamers H.</TH><TH>
SRON Laboratory for Space Research Utrecht </TH><TH>
The Winds of Early Type Supergiants </TH><TR><TH>
Lamy P.</TH><TH>
Laboratoire d'Astronomie Spatiale - Marseille </TH><TH>
Observation of Cometary Nuclei </TH><TR><TH>
Lamy P.</TH><TH>
Laboratoire d'Astronomie Spatiale - Marseille </TH><TH>
TOO: the Nucleus of a New Bright Comet </TH><TR><TH>
Langer W.</TH><TH>
Jet Propulsion Laboratory - Pasadena </TH><TH>
Evolution of Pre-Protostellar Core Fragments </TH><TR><TH>
Larson H.</TH><TH>
University of Arizona - Tucson </TH><TH>
Search for Hydrated Minerals Around 0-Rich Red Supergiants </TH><TR><TH>
Larson H.</TH><TH>
University of Arizona - Tucson </TH><TH>
Spectroscopic Studies of Volatile-Rich Asteroids </TH><TR><TH>
Laureijs R.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Dust Properties of Cirrus Heated By B-Stars </TH><TR><TH>
Laureijs R.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Properties of Peculiar Molecular Clouds At High Latitudes </TH><TR><TH>
Laureijs R.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Small Scale Structure and Dust Properties in Cloud Cores </TH><TR><TH>
Laureijs R.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Study of Dust Particles in Bright-Rimmed Clouds</TH><TR><TH>
Le Bertre T.</TH><TH>
Observatory of Paris </TH><TH>
Interstellar Dust Heated By AGB Stars </TH><TR><TH>
Le Fevre O.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
Evolution of Galaxies in Very High Redshift Clusters </TH><TR><TH>
Lecavelier A.</TH><TH>
Institut d'Astrophysique De Paris </TH><TH>
Gaseous Content of a Few Well-Known Beta Pictoris-Like Stars </TH><TR><TH>
Leech K.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
A Multiwaveband Study of the Unusual Narrow Line Quasar IRAS 20181-2244</TH><TR><TH>
Leech K.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Is There Dust in Z > 4 Quasars? </TH><TR><TH>
Leger A.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay </TH><TH>
Reflection Nebulae, Photometry and Full Range Spectroscopy </TH><TR><TH>
Leger A.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay </TH><TH>
SWS Spectrum of a Galactic Line of Sight Search for Dust and PAH
Spectral Signatures</TH><TR><TH>
Leinert C.</TH><TH>
Max-Planck-Institut Fur Astronomie - Heidelberg </TH><TH>
Mapping of COBE Fields </TH><TR><TH>
Lellouch E.</TH><TH>
Observatoire de Meudon </TH><TH>
The Surface Temperature of Pluto </TH><TR><TH>
Lemke D.</TH><TH>
Max-Planck-Institut Fuer Astronome - Heidelberg </TH><TH>
Search for Very Cold Dust Outside the Optical Disks of Galaxies </TH><TR><TH>
Liljestrom T.</TH><TH>
Helsinki University Observatory - Helsinki </TH><TH>
Heating and Cooling of Cirrus and Dark Clouds </TH><TR><TH>
Lis D.</TH><TH>
California Institute of Technology - Pasadena </TH><TH>
Star Formation in the Galactic Center Dust Ridge </TH><TR><TH>
Liseau R.</TH><TH>
Stockholm Observatory - Saltsjoebaden </TH><TH>
Class I Sources in the Galactic Giant Molecular Cloud VMR-D </TH><TR><TH>
Liseau R.</TH><TH>
Stockholm Observatory - Saltsjoebaden </TH><TH>
Spectroscopic Mapping of the Rho Ophiuchi Cloud </TH><TR><TH>
Liseau R.</TH><TH>
Stockholm Observatory - Saltsjoebaden </TH><TH>
Spectroscopic Mapping of the Serpens Cloud </TH><TR><TH>
Lisse C.</TH><TH>
NASA/GSFC - Maryland </TH><TH>
Large-Scale Observations of Scattered Sunlight and Thermal Emission
In the Tails of Bright Periodic Comets</TH><TR><TH>
Little L.</TH><TH>
University of Kent - Canterbury </TH><TH>
C+ and O Distribution in the Molecular Cloud G34.3+0.2 </TH><TR><TH>
Little L.</TH><TH>
University of Kent - Canterbury </TH><TH>
Evolutionary Status of Protostellar Condensations in L1630</TH><TR><TH>
Longair M.</TH><TH>
Cavendish Laboratory, Cambridge University </TH><TH>
Far-Infrared Photometry of Distant 3cr Radio-Galaxies </TH><TR><TH>
Lonsdale C.</TH><TH>
Infrared Processing and Analysis Center, Pasadena </TH><TH>
ISO-IRAS Faint Galaxy Survey </TH><TR><TH>
Lonsdale C.</TH><TH>
Infrared Processing and Analysis Center, Pasadena </TH><TH>
Ultraluminous High Redshift IRAS Galaxies </TH><TR><TH>
Loup C.</TH><TH>
Institut d'Astrophysique de Paris - Paris </TH><TH>
Mass-Loss and Evolution of AGB Stars in the Lmc. A Mini-Survey.</TH><TR><TH>
Lu N.</TH><TH>
IPAC/Caltech - Pasadena </TH><TH>
IRAS Galaxies With the Coldest Far-Infrared Colors </TH><TR><TH>
Lutz D.</TH><TH>
Max-Planck-Institut fuer extraterrestrische Physik - Garching </TH><TH>
Spectral Line Mapping of M82 - From Starburst to Quiescent Disk -</TH><TR><TH>
Luu J.</TH><TH>
Center for Astrophysics, Cambridge </TH><TH>
Evolution of Dust in Circumstellar Disks </TH><TR><TH>
Macchetto F.</TH><TH>
ESA / STScI Baltimore </TH><TH>
Imaging of Infrared Counter-Part of Extragalactic Radio-Jets</TH><TR><TH>
Macchetto F.</TH><TH>
ESA / STScI Baltimore </TH><TH>
Exploring the Physical Properties of the Dust Component in Early Type Galaxies</TH><TR><TH>
Madden S.</TH><TH>
NASA Ames Research Center - Moffett Field </TH><TH>
Effects of Metallicity On Star Forming Clouds in Irregular Galaxies </TH><TR><TH>
Magnier E.</TH><TH>
University of Amsterdam </TH><TH>
A Broadband Spectral Study of the Bulge of M31 </TH><TR><TH>
Maihara T.</TH><TH>
Kyoto University </TH><TH>
FIR Photometry of the Lensed Galaxy Mg0414+0534 </TH><TR><TH>
Malkan M.</TH><TH>
University of California, Los Angeles </TH><TH>
High Resolution Spectroscopy of the 2 Brightest Seyfert Nuclei </TH><TR><TH>
Manchado A.</TH><TH>
Instituto De Astrofisica De Canarias - Tenerife </TH><TH>
Spectroscopy of Heavily Obscured Post-AGB Stars </TH><TR><TH>
Martin-Pintado J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
On the Properties of the Giant Molecular Clouds in the Neutral Disk </TH><TR><TH>
Martin-Pintado J.</TH><TH>
Centro Astronomico De Yebes - Guadalajara </TH><TH>
The Physical Properties of the Stellar Winds in Selected Radio Stars</TH><TR><TH>
Marx M.</TH><TH>
Radioastronomisches Institut Der Universitaet Bonn </TH><TH>
Infrared Spectroscopy of Cool Clouds in the LMC </TH><TR><TH>
Massaro E.</TH><TH>
Istituto Astronomico, Universita` Di Roma </TH><TH>
ISO Spectroscopy of 4U 0241+61 and other Low Redshift (Z<0.1) AGNs </TH><TR><TH>
Mathieu R.</TH><TH>
University of Wisconsin - Madison </TH><TH>
Masses of Circumstellar Disks in Pre-Main-Sequence Binary Stars </TH><TR><TH>
Mathieu R.</TH><TH>
University of Wisconsin - Madison </TH><TH>
Searching for Gaps in the Disks of Pre-Main-Sequence Binary Stars </TH><TR><TH>
Matsuhara H.</TH><TH>
Department of Astrophysics, Nagoya University </TH><TH>
Far-Infrared Spectroscopy of Galactic Warm Ionized Medium </TH><TR><TH>
Mattila K.</TH><TH>
Helsinki University Observatory - Helsinki </TH><TH>
Search for Compact Very Cold Dust Clouds in the Galaxy </TH><TR><TH>
McCaughrean M.</TH><TH>
Max-Planck-Institut fuer Astronomie - Heidelberg </TH><TH>
Circumstellar Disks in the Trapezium Cluster </TH><TR><TH>
McHardy I.</TH><TH>
University of Southampton </TH><TH>
Could Emission From Dust in Clusters of Galaxies Confuse Observations
Of the Sunyaev-Zeldovich Effect?</TH><TR><TH>
McMahon R.</TH><TH>
Institute of Astronomy, Cambridge University </TH><TH>
Hyper-Luminous Infrared Galaxies </TH><TR><TH>
McMahon R.</TH><TH>
Institute of Astronomy, Cambridge University </TH><TH>
Ultraluminous High Redshift IRAS Galaxies </TH><TR><TH>
Meisenheimer K.</TH><TH>
Max-Planck-Institut fuer Astronomie - Heidelberg </TH><TH>
Mid- and Far-Infrared Polarimetry of Bright Quasars -</TH><TR><TH>
Meixner M.</TH><TH>
Dept. of Astronomy, University of Illinois </TH><TH>
FIR Imaging Dust Halos of Protoplanetary and Planetary Nebulae </TH><TR><TH>
Meixner M.</TH><TH>
Dept. of Astronomy, University of Illinois </TH><TH>
Spectroscopy of Atomic Fine Structure Lines in Evolved Stars </TH><TR><TH>
Merluzzi P.</TH><TH>
Ist. Ing. Aerospaziale Univ. Napoli </TH><TH>
Physical Properties of Dust Components in Galactic Cirrus</TH><TR><TH>
Metcalfe L.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
IR Observations of Low Surface Brightness Galaxies </TH><TR><TH>
Miley G.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Dust in the Most Distant Radio Galaxies </TH><TR><TH>
Millar T.</TH><TH>
UMIST - Manchester </TH><TH>
Carbon-Bearing Molecules in Oxygen-Rich Stars </TH><TR><TH>
Miller S.</TH><TH>
University College London - London </TH><TH>
Forbidden Rotational Specrtum of H3+ in the Ionosphere of Jupiter</TH><TR><TH>
Mirabel F.</TH><TH>
Service d'Astrophysique. CEA-Saclay </TH><TH>
Clusters of Galaxies At Early Epochs of the Universe </TH><TR><TH>
Mirabel F.</TH><TH>
Service d'Astrophysique. CEA-Saclay </TH><TH>
The Galactic Superluminal Source Grs 1915+105 </TH><TR><TH>
Mittaz J.</TH><TH>
Department of Space and Climate Physics, UCL </TH><TH>
FIR Observation of X-Ray Selected Emission Line Galaxies From
The Rixos Survey</TH><TR><TH>
Mobasher B.</TH><TH>
Imperial College, London </TH><TH>
Photometry of Galaxies in Deep Radio-Selected Surveys </TH><TR><TH>
Mochizuki K.</TH><TH>
Institute of Space and Astronautical Science. Kanagawa </TH><TH>
FIR Spectroscopy of M31 Seach for [C II] Deficit</TH><TR><TH>
Mochizuki K.</TH><TH>
Institute of Space and Astronautical Science. Kanagawa </TH><TH>
FIR Spectroscopy of M33 Interstellar Physics in a Low Metal Spiral</TH><TR><TH>
Molinari S.</TH><TH>
Istituto di Radioastronomia - CNR - Bologna </TH><TH>
Spectroscopy of Candidate Progenitors of Ultracompact HII Regions</TH><TR><TH>
Montesinos B.</TH><TH>
LAEFF - Madrid </TH><TH>
The Infrared Energy Distribution of FG Sge </TH><TR><TH>
Montmerle T.</TH><TH>
Service d'Astrophysique - CEA Saclay </TH><TH>
Search for H2 and H3+ IR Lines Associated With X-Ray Sources Embedded in
Molecular Clouds</TH><TR><TH>
Montmerle T.</TH><TH>
Service d'Astrophysique - CEA Saclay </TH><TH>
Spectral Features of X-Ray Irradiated Dust </TH><TR><TH>
Moorwood A.</TH><TH>
ESO - Garching </TH><TH>
Energy Source in Ultraluminous Infrared Galaxies. Starbursts Or Obscured
AGN'S in IRAS Galaxies</TH><TR><TH>
Moran J.</TH><TH>
Harvard-Smithsonian CfA, Cambridge </TH><TH>
High Spectral Resolution Observations of Megamaser Galaxies </TH><TR><TH>
Moritz P.</TH><TH>
Radioastronomisches Institut Der Universitaet Bonn </TH><TH>
Infrared Photometrie and Spectroscopy of the Draco Nebula </TH><TR><TH>
Morris M.</TH><TH>
UCLA, Los Angeles </TH><TH>
Thermal Water Line Emission From Warm Clouds Near the Galactic Center </TH><TR><TH>
Mouri H.</TH><TH>
Meteorological Research Institute - Tsukuba </TH><TH>
MIR Spectroscopy of Heavily Obscured IRAS Galaxies </TH><TR><TH>
Muller C.</TH><TH>
Belgian Institute for Space Aeronomy - Brussels </TH><TH>
TOO: Martian Dust Storms Observations. </TH><TR><TH>
Myers P.</TH><TH>
Smithonian Astrophysical Observatory, Cambridge </TH><TH>
Warm Dust Imaging of Nearby Low Mass Protostars </TH><TR><TH>
Nakagawa T.</TH><TH>
Institute of Space and Astronautical Science. Kanagawa </TH><TH>
IRTs Follow-On Observation of SNR'S With FIR Fine Structure Lines </TH><TR><TH>
Nakajima T.</TH><TH>
CALTECH, Pasadena </TH><TH>
A Search for Brown Dwarf Companions to Young Nearby Stars </TH><TR><TH>
Naylor D.</TH><TH>
University of Lethbridge, Alberta </TH><TH>
LWS Grating Observations of HD On Uranus and Neptune </TH><TR><TH>
Naylor T.</TH><TH>
Keele University, Staffordshire </TH><TH>
TOO: Observations of Low-Mass X-Ray Binaries</TH><TR><TH>
Neininger N.</TH><TH>
IRAM - St-Martin-d'Heres </TH><TH>
Mapping the Surroundings of NGC 206 </TH><TR><TH>
Neininger N.</TH><TH>
IRAM - St-Martin-d'Heres </TH><TH>
Polarimetric Mapping of the Central Region of M82 </TH><TR><TH>
Neri R.</TH><TH>
IRAM - St-Martin-d'Heres </TH><TH>
A Key Spectroscopic Study of Crl2688, Crl618 and NGC7027 </TH><TR><TH>
Neufeld D.</TH><TH>
Johns Hopkins University - Baltimore </TH><TH>
Search for Far-IR Transitions of Interstellar Hydrogen Halides </TH><TR><TH>
Neufeld D.</TH><TH>
Johns Hopkins University - Baltimore </TH><TH>
Search for Ultra-High-Excitation Rotational Lines of Water </TH><TR><TH>
Nguyen-Rieu Q.</TH><TH>
Observatoire De Paris, Demirm - Paris </TH><TH>
Water Abundance in the Envelope of Optical Oxygen-Rich AGB Stars </TH><TR><TH>
Nisini B.</TH><TH>
CNR Istituto Di Fisica Dello Spazio Interplanetario, Frascati </TH><TH>
Spectroscopic Imaging of Bipolar Outflows </TH><TR><TH>
Noriega-Crespo A. </TH><TH>
IPAC, California </TH><TH>
Momentum Injection in Molecular Outflows. Imaging in H2 and Spectroscopy
Scanning in [OI]</TH><TR><TH>
Odenwald S.</TH><TH>
Applied Research Corporation - Landover, Maryland </TH><TH>
Why Is the Comet-Shaped Cloud, NGC 5367 Forming Stars? </TH><TR><TH>
Oestreicher M.</TH><TH>
Astronomical Institute Ruhr-University Bochum </TH><TH>
Broadband and Spectrophotometry of Luminous Stars in the Lmc </TH><TR><TH>
Okumura K.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay Cedex </TH><TH>
Diffuse Interstellar Medium in the Magellanic Clouds </TH><TR><TH>
Oldham P.</TH><TH>
Queen Mary and Westfield College - London </TH><TH>
FIR Spectroscopy and Mapping of the W3 Region the Nature of Irs4s.</TH><TR><TH>
Oliva E.</TH><TH>
Arcetri Observatory - Firenze </TH><TH>
Probing Cool Molecular/Atomic Gas in Cooling Flow Cd Galaxies. </TH><TR><TH>
Oliver S.</TH><TH>
Imperial College, London </TH><TH>
Evolution in the SED of Ultraluminous IRAS Galaxies </TH><TR><TH>
Omont A.</TH><TH>
Institut d'Astrophysique De Paris </TH><TH>
ISOCAM Survey of the Inner Galaxy </TH><TR><TH>
Onaka T.</TH><TH>
Department of Astronomy, University of Tokyo </TH><TH>
A Systematic Study of Infrared Emission From Galaxies </TH><TR><TH>
Onaka T.</TH><TH>
Department of Astronomy, University of Tokyo </TH><TH>
FIR Polarization of Diffuse Thermal Emission </TH><TR><TH>
Onaka T.</TH><TH>
Department of Astronomy, University of Tokyo </TH><TH>
Time Variation of Circumstellar Envelopes </TH><TR><TH>
Onishi T.</TH><TH>
Nagoya University - Nagoya </TH><TH>
Deep IR Observations of Starless Cores in Taurus B213 Region </TH><TR><TH>
Osip D.</TH><TH>
University of Florida - Gainesville </TH><TH>
Spectral Analysis of Carbon-Chain Depleted Comets. </TH><TR><TH>
Oudmaijer R.</TH><TH>
Kapteyn Laboratory Groningen </TH><TH>
Is Wra1484 a Hot Post-AGB Star? </TH><TR><TH>
Oudmaijer R.</TH><TH>
Kapteyn Laboratory Groningen </TH><TH>
Post-AGB Stars With Cool Dustshells </TH><TR><TH>
Padovani P.</TH><TH>
Physics Department, II University of Rome </TH><TH>
ISO Observations of Radio-Selected Bl Lacs </TH><TR><TH>
Pauls T.</TH><TH>
Naval Research Laboratory - Washington </TH><TH>
Far-Infrared Spectroscopy of G159.6-18.5 </TH><TR><TH>
Penny A.</TH><TH>
Rutherford Appleton Laboratory - Didcot </TH><TH>
Dust in Globular Clusters </TH><TR><TH>
Perault M.</TH><TH>
Ecole Normale Superieure - Paris </TH><TH>
Photo-Imaging of Quiescent Molecular Clouds in the Inner Galaxy </TH><TR><TH>
Perez-Fournon I.</TH><TH>
Instituto de Astrofisica de Canarias, Tenerife </TH><TH>
Search for Hidden BLR in Seyfert 2 Galaxies </TH><TR><TH>
Pfau W.</TH><TH>
Jena University Observatory - Jena </TH><TH>
The Signature of Diffuse Interstellar Bands in Mid Infrared Emission </TH><TR><TH>
Phillips T.</TH><TH>
California Institute of Technology - Pasadena </TH><TH>
Oxygen in Molecular Clouds </TH><TR><TH>
Pierre M.</TH><TH>
Service d'Astrophysique, CE Saclay - Gif sur Yvette </TH><TH>
Detailed Insights Into the Intra-Cluster Medium of Abell 2256 </TH><TR><TH>
Poglitsch A.</TH><TH>
MPE - Garching </TH><TH>
Spectral Line Mapping and the Extended Medium in nearby Galaxies </TH><TR><TH>
Prieto A.</TH><TH>
MPE,Rosat Division - Garching </TH><TH>
Anisotropy of the Radiation in NGC 5252 </TH><TR><TH>
Prusti T.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Bolometric Luminosity Functions of nearby Star Forming Regions </TH><TR><TH>
Prusti T.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Extended Infrared Emission Around Young Stars </TH><TR><TH>
Prusti T.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Search of the Comet-Like Activity in Stars With Non-Periodic Algol-Type Minima</TH><TR><TH>
Prusti T.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
TOO: Evolution of the Circumstellar Environment During An Fu Ori or
Ex Lup Outburst</TH><TR><TH>
Prusti T.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Variable Infrared Emission From Circumstellar Environment of Young
Intermediate Mass Stars</TH><TR><TH>
Prusti T.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Spectral Energy Distributions of Young Stellar Objects </TH><TR><TH>
Puget J.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay </TH><TH>
Deep Survey At 4.5 Micron Spectrum of Faint Galaxies in the Near IR
Cosmological Window</TH><TR><TH>
Puget J.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay </TH><TH>
Spectral Survey of the Cold Interstellar Medium </TH><TR><TH>
Puxley P.</TH><TH>
Royal Observatory Edinburgh </TH><TH>
Mid-IR Recombination Line Spectroscopy of Bright Galaxies </TH><TR><TH>
Puxley P.</TH><TH>
Royal Observatory Edinburgh </TH><TH>
The Dust Content of HII Regions </TH><TR><TH>
Quirrenbach A.</TH><TH>
MPE, Garching </TH><TH>
Absorption Lines Towards the Nucleus of Centaurus A </TH><TR><TH>
Quirrenbach A.</TH><TH>
MPE, Garching </TH><TH>
Rapid Infrared Variability of An Extreme BL Lac Object </TH><TR><TH>
Ramsay G.</TH><TH>
Mullard Space Science Lab/University Collge London </TH><TH>
Observations of Magnetic CVs. The Determination of Magnetic Field Strengths</TH><TR><TH>
Rasmussen I.</TH><TH>
Danish Space Research Institute - Lyngby </TH><TH>
Shock Processing of Dust in Tycho's SNR </TH><TR><TH>
Rawlings S.</TH><TH>
Oxford University - Oxford </TH><TH>
Far-IR Photometry of High-Redshift Radioquasars </TH><TR><TH>
Rawlings S.</TH><TH>
Oxford University - Oxford </TH><TH>
Far-IR Photometry of Radio Quiet Quasars </TH><TR><TH>
Reach W.</TH><TH>
NASA/GSFC - Greenbelt </TH><TH>
Grain Destruction in Intermediate-Velocity Clouds </TH><TR><TH>
Reach W.</TH><TH>
NASA/GSFC - Greenbelt </TH><TH>
Infrared Emission From the Warm Ionized Medium </TH><TR><TH>
Reach W.</TH><TH>
NASA/GSFC - Greenbelt </TH><TH>
Phase Transitions in Translucent Clouds </TH><TR><TH>
Reach W.</TH><TH>
NASA/GSFC - Greenbelt </TH><TH>
Supernova Interactions With Molecular Clouds and their influnce on
X-Ray Remnant Morphology</TH><TR><TH>
Reid I.</TH><TH>
California Institute of Technology - Pasadena </TH><TH>
Cocoon Stars in the Magellanic Clouds </TH><TR><TH>
Reinsch K.</TH><TH>
Universitaets-Sternwarte Goettingen </TH><TH>
Cyclotron Spectroscopy of Magnetic Cataclysmic Variables </TH><TR><TH>
Rengarajan T.</TH><TH>
Tata Institute of Fundamental Research - Bombay </TH><TH>
Infrared Emission From Rs Cvn Binaries </TH><TR><TH>
Renzini A.</TH><TH>
Dept. of Astronomy, University of Bologna </TH><TH>
FIR Emission in X-Ray Bright and X-Ray Faint Early-Type Galaxies. </TH><TR><TH>
Richards P.</TH><TH>
Rutherford Appleton Laboratories - Didcot </TH><TH>
Dust in Galactic Open Clusters </TH><TR><TH>
Rieke G.</TH><TH>
Steward Observatory - Tucson </TH><TH>
Low Mass Pleiades Brown Dwarfs </TH><TR><TH>
Rieke G.</TH><TH>
Steward Observatory - Tucson </TH><TH>
Optically Quiet QSOs </TH><TR><TH>
Rieke G.</TH><TH>
Steward Observatory - Tucson </TH><TH>
Star Formation and Evolution of Seyfert Nuclei </TH><TR><TH>
Rieke M.</TH><TH>
Steward Observatory - Tucson </TH><TH>
Mid-Infrared Output of Quiescent Galaxies </TH><TR><TH>
Rieke M.</TH><TH>
Steward Observatory - Tucson </TH><TH>
Study of the Far-IR Properties of BAL QSOs </TH><TR><TH>
Roche P.</TH><TH>
Oxford University - Oxford </TH><TH>
Dust Emission Features in Stellar Envelopes </TH><TR><TH>
Roche P.</TH><TH>
Oxford University - Oxford </TH><TH>
Magnetic Field Structures in Star Forming Regions </TH><TR><TH>
Rodono` M.</TH><TH>
Catania Astrophysical Observatory, Catania </TH><TH>
Infrared Excess in RS CVN and Algol Type Binaries </TH><TR><TH>
Rodono` M.</TH><TH>
Catania Astrophysical Observatory, Catania </TH><TH>
Infrared Excess in Dme Stars </TH><TR><TH>
Rouan D.</TH><TH>
Observatoire de Paris-Meudon </TH><TH>
PAHs/Very Small Grains in Edge-On Galaxies </TH><TR><TH>
Rowan-Robinson M.</TH><TH>
Imperial College, London </TH><TH>
A Deep Large-Area Survey With ISO in Open Time </TH><TR><TH>
Rowan-Robinson M.</TH><TH>
Imperial College, London </TH><TH>
Photometric Identification of High Redshift Objects From IRAS FSS Blank Fields</TH><TR><TH>
Rowan-Robinson M.</TH><TH>
Imperial College, London </TH><TH>
Photometry and Spectroscopy of Ultraluminous IRAS Galaxies: the QDOT Sample</TH><TR><TH>
Rubin R.</TH><TH>
NASA Ames Research Center (Orion Enterprises) </TH><TH>
An Analysis of Planetary Nebulae: Temperatures, Densities, and Abundances</TH><TR><TH>
Rubin R.</TH><TH>
NASA Ames Research Center (Orion Enterprises) </TH><TH>
Iron Abundances in Gaseous Nebulae </TH><TR><TH>
Russell S.</TH><TH>
Dublin Institute for Advanced Studies </TH><TH>
A Statistical Study of Dust in Magellanic Cloud Supernova Remnants </TH><TR><TH>
Russell S.</TH><TH>
Dublin Institute for Advanced Studies </TH><TH>
A Statistical Study of the SEDs of Very Cold IRAS Sources</TH><TR><TH>
Russell S.</TH><TH>
Dublin Institute for Advanced Studies </TH><TH>
The Energy Sources of Molecular Outflows </TH><TR><TH>
Sahai R.</TH><TH>
Jet Propulsion Laboratory, Caltech </TH><TH>
Far-IR Spectroscopy of Very Young, Low-Excitation Planetary Nebulae </TH><TR><TH>
Salama A.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Unravelling the Murky Past of the Old Nova Gk Per </TH><TR><TH>
Sams B.</TH><TH>
Max Planck Institute Ex - Garching </TH><TH>
The Power Source of High-Z Ultraluminous Galaxies </TH><TR><TH>
Sanders D.</TH><TH>
Institute for Astronomy - Honolulu </TH><TH>
Complete (PHT32-C200) Maps of a Nearby Prototypical GMC </TH><TR><TH>
Sandford S.</TH><TH>
NASA/Ames Research Center - Moffett Field </TH><TH>
A Search for Solid State Ozone (O3) in the Ices in Interstellar
Dense Molecular Clouds</TH><TR><TH>
Sandford S.</TH><TH>
NASA/Ames Research Center - Moffett Field </TH><TH>
The 11-16 Micron C-H Bending Modes of Interstellar PAHs </TH><TR><TH>
Sandford S.</TH><TH>
NASA/Ames Research Center - Moffett Field </TH><TH>
The Composition of the H2-Containing Ice and Dust Along the Line of
Sight to the Unique Object Wl5</TH><TR><TH>
Sauvage M.</TH><TH>
Service d'Astrophysique, CEA-Saclay </TH><TH>
Hot Dust in the Central Regions of Early-Type Galaxies? </TH><TR><TH>
Schmitt B.</TH><TH>
LGGE - CNRS - Saint Martin d'Heres </TH><TH>
The Composition and Temperature of the Surface of Io </TH><TR><TH>
Schulte-Ladbeck R.</TH><TH>
University of Pittsburgh - Pittsburgh </TH><TH>
Asymmetric Mass Loss in the Upper HR Diagram - the Role of Molecular CO</TH><TR><TH>
Schultz A.</TH><TH>
NASA-AMES Research Lab - Moffett Field </TH><TH>
Imaging of Shocked Molecular Hydrogen in Herbig-Haro Objects </TH><TR><TH>
Schulz R.</TH><TH>
Max-Planck-Institut Fuer Aeronomie, Lindau </TH><TH>
Distributed Sources in Cometary Comae Column Density Profiles of Parent
Potential Parent Molecules</TH><TR><TH>
Schutte W.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
IR Absorption Features of H2O Diluted in Apolar Ices </TH><TR><TH>
Schutte W.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
IR Absorption Features of Nitrogen and Sulfur Containing Molecules in
Interstellar Ices</TH><TR><TH>
Scotti J.</TH><TH>
University of Arizona - Tucson </TH><TH>
Characterization of the Size of Short-Period Comet Nuclei. </TH><TR><TH>
Scoville N.</TH><TH>
California Institute of Technology - Pasadena </TH><TH>
ISO Search for H2 Rotational Transitions in High Z Quasars/Host Galaxies</TH><TR><TH>
Sedlmayr E.</TH><TH>
Institut fuer Astronomie und Astrophysik - Berlin </TH><TH>
Variability of Circumstellar Dust Shells around long--period variables</TH><TR><TH>
Sellgren K.</TH><TH>
Astronomy Department, Ohio State University </TH><TH>
Imaging of Infrared Emission Features in Reflection Nebulae </TH><TR><TH>
Serra G.</TH><TH>
CESR / CNRS - Toulouse cedex </TH><TH>
IR Emission of SZ Galaxy Clusters </TH><TR><TH>
Shanks T.</TH><TH>
Physics Department, Durham University </TH><TH>
Infra-Red Properties of X-Ray Selected Qsos and Galaxies </TH><TR><TH>
Shields J.</TH><TH>
Steward Observatory - Tucson </TH><TH>
Infrared Spectroscopy of the Lowest Luminosity Seyfert 1 Nucleus</TH><TR><TH>
Sibille F.</TH><TH>
Observatoire De Lyon - Saint Genis Laval </TH><TH>
Luninosity Functions of Low Mass Star in Nearby Molecular Clouds </TH><TR><TH>
Siebenmorgen R.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
Dust Emission of Reflection Nebulae </TH><TR><TH>
Siebenmorgen R.</TH><TH>
ISO Science Operations, ESTEC, Noordwijk </TH><TH>
The Energetics of Extended Emission Around Herbig He/Be Stars </TH><TR><TH>
Simpson C.</TH><TH>
Oxford University - Oxford </TH><TH>
Direct Observations of the Broad Line Region in Cygnus A </TH><TR><TH>
Skinner C.</TH><TH>
Lawrence Livermore National Laboratory </TH><TH>
Co Observations of Mass-Loss in Low-Mass Post-Main Sequence Stars </TH><TR><TH>
Skinner C.</TH><TH>
Lawrence Livermore National Laboratory </TH><TH>
PAHs and Chromospheres in M-Supergiants </TH><TR><TH>
Smith B.</TH><TH>
University of Texas - Austin </TH><TH>
Mid-Infrared Spectral Imaging of Galaxy Bulges </TH><TR><TH>
Smith B.</TH><TH>
University of Texas - Austin </TH><TH>
The ISM in Low Luminosity Virgo Cluster Spiral Galaxies </TH><TR><TH>
Smith H.</TH><TH>
Laboratory for Astrophysics - Washington DC </TH><TH>
Excitation and Kinematics of Sgr A* </TH><TR><TH>
Smith M.</TH><TH>
MPIA, Heidelberg </TH><TH>
Molecular Hydrogen in Bipolar Outflows </TH><TR><TH>
Soifer B.</TH><TH>
California Institute of Technology - Pasadena </TH><TH>
ISO/SWS Observations of Ultraluminous Infrared Galaxies </TH><TR><TH>
Spaans M.</TH><TH>
Sterrewacht Leiden - Leiden </TH><TH>
FIR Line Observations of Photon Dominated Regions Around Cool Stars </TH><TR><TH>
Spear G.</TH><TH>
Sonoma State University - Rohnert Park </TH><TH>
The Period-Luminosity Relationship at 12 Microns for LMC Cepheids </TH><TR><TH>
Spinoglio L.</TH><TH>
Istituto di Fisica dello Spazio Interplanetario, Frascati </TH><TH>
IR Energy Distributions and Imaging of the Complete Sample of 12 micron AGN </TH><TR><TH>
Spinrad H.</TH><TH>
University of California, Berkeley </TH><TH>
Mg1019+0535: A Dusty, High-Z Radio Galaxy </TH><TR><TH>
Spyromilio J.</TH><TH>
ESO - Garching </TH><TH>
IR Studies of Extremely Young Supernova Remnants Mid-IR Supernova Studies</TH><TR><TH>
Stacey G.</TH><TH>
Cornell University - Ithaca, NY </TH><TH>
The Mid-IR Spectral Energy Distribution of IR Luminous Galaxies </TH><TR><TH>
Stapelfeldt K.</TH><TH>
Jet Propulsion Laboratory - Pasadena </TH><TH>
Dissipation of Gaseous Circumstellar Disks </TH><TR><TH>
Stark R.</TH><TH>
Ecole Normale Superieure - Paris </TH><TH>
Cooling By the Diffuse Cold and Warm Phases of the ISM </TH><TR><TH>
Stark R.</TH><TH>
Ecole Normale Superieure - Paris </TH><TH>
The Gas-Dust Connection and Cooling in Proto-Planetary Discs </TH><TR><TH>
Stauffer J.</TH><TH>
Center for Astrophysics, Cambridge </TH><TH>
Dust Around `A' Stars in Young Open Clusters </TH><TR><TH>
Stauffer J.</TH><TH>
Center for Astrophysics, Cambridge </TH><TH>
Dust Around Solar-Type Stars in Young Open Clusters </TH><TR><TH>
Steele I.</TH><TH>
Leicester University - Leicester </TH><TH>
Photometry of Cluster Low Mass Stars and Brown Dwarfs </TH><TR><TH>
Stern A.</TH><TH>
Southwest Research Institute - San Antonio, Texas </TH><TH>
A Comprehensive Investigation of the Thermal Properties and Rotational
Thermal Variability of the Pluto-Charon Binary and Chiron</TH><TR><TH>
Sternberg A.</TH><TH>
MPIE, Garching </TH><TH>
Mid-Infrared Spectroscopy of Liners - the AGN Connection </TH><TR><TH>
Sternberg A.</TH><TH>
MPIE, Garching </TH><TH>
[FeII] Emission in Starburst Galaxies and Active Galactic Nuclei </TH><TR><TH>
Stockton A.</TH><TH>
Institute for Astronomy, Univerity of Hawaii </TH><TH>
Correlations Between FIR Spectra and Qso Host Galaxy Morphology </TH><TR><TH>
Strazzulla G.</TH><TH>
Istituto Di Astronomia Universita' Di Catania </TH><TH>
Amorphous vs Crystalline Water Ice Ice Structure in Circumstellar Envelopes</TH><TR><TH>
Stutzki J.</TH><TH>
I. Physikalisches Institut der Universitaet zu Koeln </TH><TH>
High Density PDR Tracers </TH><TR><TH>
Stutzki J.</TH><TH>
I. Physikalisches Institut der Universitaet zu Koeln </TH><TH>
The Changing Faces of PDRs </TH><TR><TH>
Stutzki J.</TH><TH>
I. Physikalisches Institut der Universitaet zu Koeln </TH><TH>
Trace Species Detected Through PDR Emission </TH><TR><TH>
Sugai H.</TH><TH>
Dept. of Astron., UCLA </TH><TH>
Energy Sources for Emission Lines From Liners </TH><TR><TH>
Sulentic J.</TH><TH>
University of Alabama - Tuscaloosa </TH><TH>
Star Formation and Secular Evolution in Galaxies Mixed Morphology Pairs</TH><TR><TH>
Tagliaferri G.</TH><TH>
Osservatorio Astronomico di Brera Merate </TH><TH>
Infrared Continuum Variability of the highly variable BL Lac object Pks2155-304</TH><TR><TH>
Tanabe T.</TH><TH>
Institute of Astronomy, the University of Tokyo </TH><TH>
A Systematic Study of Unidentified Features in AGB Stars </TH><TR><TH>
Tanabe T.</TH><TH>
Institute of Astronomy, the University of Tokyo </TH><TH>
A Systematic Study On the Properties of Dust Grains Around M Supergiant Stars</TH><TR><TH>
Tanabe T.</TH><TH>
Institute of Astronomy, the University of Tokyo </TH><TH>
Spectrophotometric Observations of AGB Stars in the Magellanic Clouds </TH><TR><TH>
Tanabe T.</TH><TH>
Institute of Astronomy, the University of Tokyo </TH><TH>
TOO: Dust Formation Around R CRB Type Stars At their Minimums </TH><TR><TH>
Taniguchi Y.</TH><TH>
Tohoku University - Sendai </TH><TH>
Star Formation in Hyperluminous Infrared Galaxies </TH><TR><TH>
Tauber J.</TH><TH>
ESA SSD, Noordwijk </TH><TH>
Galactic Distribution of the Isotopic Ratio (13)CII/CII </TH><TR><TH>
Tauber J.</TH><TH>
ESA SSD, Noordwijk </TH><TH>
Observations of High-J CO Lines in Dense Photon Dominated Regions </TH><TR><TH>
Tedesco E.</TH><TH>
Mission Research Corporation - Nashua, NH </TH><TH>
Asteroid Size-Frequency Distribution </TH><TR><TH>
Thomas N.</TH><TH>
Max-Planck-Institut Fuer Aeronomie, Lindau </TH><TH>
Io's SO2 Atmosphere and Torus </TH><TR><TH>
Thum C.</TH><TH>
IRAM - St. Martin d`Heres </TH><TH>
The Disk of MWC349 </TH><TR><TH>
Thum C.</TH><TH>
IRAM - St. Martin d`Heres </TH><TH>
The Recombination Line Maser </TH><TR><TH>
Tilgner C.</TH><TH>
Max-Planck-Institut Fuer AStronomie - Heidelberg </TH><TH>
SETI: Search for Dyson Spheres </TH><TR><TH>
Tinney C.</TH><TH>
European Southern Observatory - Garching </TH><TH>
The Near- and Far-Infrared Spectra of Very Late M-Stars </TH><TR><TH>
Treves A.</TH><TH>
SISSA/ISAS,Trieste - Trieste </TH><TH>
The Infrared Energy Distribution of the BL Lac Object PKS 2155-304 </TH><TR><TH>
Tsuji T.</TH><TH>
Institute of Astronomy, the University of Tokyo </TH><TH>
High Resolution Spectroscopy of Co and Sio in Red (Super)Giants </TH><TR><TH>
Tsuji T.</TH><TH>
Institute of Astronomy, the University of Tokyo </TH><TH>
Infrared Excesses in Carbon Stars of the Galactic Halo and the Lmc </TH><TR><TH>
Tsuji T.</TH><TH>
Institute of Astronomy, the University of Tokyo </TH><TH>
Infrared Properties of Very Low Mass Stars From M Dwarfs to Brown Dwarfs</TH><TR><TH>
Tuffs R.</TH><TH>
MPIK, Heidelberg </TH><TH>
Polarimetric Imaging of MIR Synchrotron Emission in Cas A </TH><TR><TH>
Tuffs R.</TH><TH>
MPIK, Heidelberg </TH><TH>
Polarimetric Mapping of Synchrotron Emission in the Crab Nebula </TH><TR><TH>
Turner J.</TH><TH>
UCLA - Los Angeles </TH><TH>
Gas and Dust Properties in Two Nearby Spiral Galaxies </TH><TR><TH>
Van Buren D.</TH><TH>
IPAC - Pasadena </TH><TH>
ISOCAM Search for Pulsar Debris Disks </TH><TR><TH>
Van Buren D.</TH><TH>
IPAC - Pasadena </TH><TH>
Infrared Coronal Lines in Ultracompact HII Regions </TH><TR><TH>
Van Buren D.</TH><TH>
IPAC - Pasadena </TH><TH>
Stellar Wind Bow Shocks - Laboratories for Dust Shock Processing </TH><TR><TH>
Van De Steene G.</TH><TH>
Kapteyn Astronomical Institute - Groningen </TH><TH>
Accurate Abundance Determination of CNO in PN. </TH><TR><TH>
Van Der Hucht K.</TH><TH>
Sron-Utrecht </TH><TH>
Neon Abundance in Wolf-Rayet Stellar Winds </TH><TR><TH>
Van Der Hulst J.</TH><TH>
Kapteyn Astronomical Institute - Groningen </TH><TH>
Density and Ionization Structure of HII Regions </TH><TR><TH>
Van Der Hulst J.</TH><TH>
Kapteyn Astronomical Institute - Groningen </TH><TH>
Dust in Shell Galaxies </TH><TR><TH>
Van Der Hulst J.</TH><TH>
Kapteyn Astronomical Institute - Groningen </TH><TH>
Dust Temperatures in Galaxies as Function of their Surface Brightness</TH><TR><TH>
Van Der Veen W.</TH><TH>
Columbia University, New York </TH><TH>
Imaging of Dust Shells Around AGB and Post-AGB Stars </TH><TR><TH>
Van Der Werf P.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Pressure in the Interstellar Medium of M33 </TH><TR><TH>
Van Der Werf P.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Pressure in the Interstellar Medium of Late-Type Galaxies </TH><TR><TH>
Van Der Werf P.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
Spectroscopy of Distant Radio Galaxies: Starbursts and Active Nuclei at redshift
1</TH><TR><TH>
Van Dishoeck E.</TH><TH>
Leiden Observatory - Leiden </TH><TH>
The Chemical State of Southern High-Mass Star-Forming Regions </TH><TR><TH>
Veilleux S.</TH><TH>
Kitt Peak National Observatory - Tucson </TH><TH>
Infrared Spectroscopy of a Unbiased Sample of Ultraluminous IRAS Galaxies
With Log[L_{IR}/L_{Sun}] = 12.3 - 13.0 and Z = 0.1 - 0.3.</TH><TR><TH>
Verheijen M.</TH><TH>
Kapteyn Astronomical Institute - Groningen </TH><TH>
An Improved Distance Indicator for Spiral Galaxies </TH><TR><TH>
Verstraete L.</TH><TH>
Institut d'Astrophysique Spatiale - Orsay </TH><TH>
Mid-IR Spectroscopy of Small Dust Grains Around Hot Stars </TH><TR><TH>
Vigotti M.</TH><TH>
Istituto Di Radioastronomia C.N.R. Bologna </TH><TH>
The Nature of AGN and Stellar Populations in High Z Powerful Radio Galaxies</TH><TR><TH>
Vogel M.</TH><TH>
Institute of Astronomy - Zurich </TH><TH>
Dust in Symbiotic Binaries. </TH><TR><TH>
Volk K.</TH><TH>
University of Calgary, Alberta </TH><TH>
Spectroscopy of Featureless, Low-Temperature IRAS Sources </TH><TR><TH>
Volk K.</TH><TH>
University of Calgary, Alberta </TH><TH>
Study of Unusual 11.3 Micron Feature Sources </TH><TR><TH>
Volk K.</TH><TH>
University of Calgary, Alberta </TH><TH>
Study of An Unknown Type of Dust </TH><TR><TH>
Waelkens C.</TH><TH>
Instituut Voor Sterrenkunde - Leuven </TH><TH>
Circumstellar Matter Around High-Latitude Supergiants </TH><TR><TH>
Waelkens C.</TH><TH>
Instituut Voor Sterrenkunde - Leuven </TH><TH>
Dust Discs Around Young Main-Sequence Stars </TH><TR><TH>
Waelkens C.</TH><TH>
Instituut Voor Sterrenkunde - Leuven </TH><TH>
Monitoring of the IR Emission of HR4049 and HD213985 </TH><TR><TH>
Waelkens C.</TH><TH>
Instituut Voor Sterrenkunde - Leuven </TH><TH>
Probing the Vega Phenomenon in Open Clusters </TH><TR><TH>
Walker C.</TH><TH>
Steward Observatory - Tucson </TH><TH>
[C II] Emission as a Probe of Starformation in Absorption Line Systems </TH><TR><TH>
Walker H.</TH><TH>
DRAL - Didcot </TH><TH>
Mapping of R CRB Dust Shells </TH><TR><TH>
Walker H.</TH><TH>
DRAL - Didcot </TH><TH>
Mapping the Environment of Vega-Like Stars </TH><TR><TH>
Walmsley C.</TH><TH>
Max Planck Institut fuer Radioastronomie, Bonn. </TH><TH>
Observation of NH3 in Some Hot Molecular Cores </TH><TR><TH>
Ward M.</TH><TH>
Oxford University </TH><TH>
Centaurus A: Qu'Est-Ce Que C'Est? </TH><TR><TH>
Ward M.</TH><TH>
Oxford University </TH><TH>
Hot Dust in High Redshift Quasars? Implications for the Presence/Absence of Tori</TH><TR><TH>
Ward M.</TH><TH>
Oxford University </TH><TH>
IRAS F10214+4724: Starburst Or Enshrouded Quasar? </TH><TR><TH>
Ward-Thompson D.</TH><TH>
Royal Observatory Edinburgh - Edinburgh </TH><TH>
Pre-Protostellar Cores</TH><TR><TH>
Waters L.</TH><TH>
Astronomical Institute, Amsterdam </TH><TH>
IR Photometry of K Stars with IR excess. The Nature of Circumstellar dust in K Giants</TH><TR><TH>
Waters L.</TH><TH>
Astronomical Institute, Amsterdam </TH><TH>
Infrared Spectroscopy of Normal O and B Stars: </TH><TR><TH>
</TH><TH> </TH><TH>A Search for Low-Density Circumstellar Gas</TH><TR><TH>
Waters L.</TH><TH>
Astronomical Institute, Amsterdam </TH><TH>
Massive Stars in the LMC and SMC: </TH><TR><TH>
</TH><TH> </TH><TH>A Study of the Ejecta of B[E] Stars in the Magellanic Clouds</TH><TR><TH>
Wehrse R.</TH><TH>
Institut f. Theoret. Astrophysik, Univ. Heidelberg </TH><TH>
Temperature Stratification in Cool Dwarf Atmospheres </TH><TR><TH>
Weinberger R.</TH><TH>
Institut fuer Astronomie Innbruck </TH><TH>
Dust in Born-Again Planetary Nebulae </TH><TR><TH>
Weinberger R.</TH><TH>
Institut fuer Astronomie Innbruck </TH><TH>
Edge-On Dust Disks in Planetary Nebulae </TH><TR><TH>
Weiss W.</TH><TH>
Institute for Astronomy, Vienna </TH><TH>
Dust and Gas Environment of Lambda-Bootis Stars </TH><TR><TH>
Wendker H.</TH><TH>
Hamburger Sternwarte - Hamburg </TH><TH>
G 79.29+0.46: A New LBV and its Shell. </TH><TR><TH>
Wennmacher A.</TH><TH>
Radioastronomisches Institut der Universitaet Bonn </TH><TH>
Physical Properties of a Cloud Located in the Local Hot Bubble </TH><TR><TH>
Werner M.</TH><TH>
JPL, Pasadena </TH><TH>
Studies of Wolf-Rayet Galaxies </TH><TR><TH>
Wesselius P.</TH><TH>
SRON Space Laboratory Groningen </TH><TH>
CO2 and CH4 Ice Absorption Features </TH><TR><TH>
White D.</TH><TH>
Institute of Astronomy, Cambridge </TH><TH>
Dust in the Stripped Interstellar Medium of M86. </TH><TR><TH>
Whitelock P.</TH><TH>
ESO, Garching </TH><TH>
A Study of M Stars With Unusual Mass-Loss Rates </TH><TR><TH>
Whitelock P.</TH><TH>
ESO, Garching </TH><TH>
Mass-Loss History of the Lithium-Rich S Star Rz Sgr </TH><TR><TH>
Wiklind T.</TH><TH>
Onsala Space Observatory </TH><TH>
Dust and Gas Properties of Dwarf Elliptical Galaxies. </TH><TR><TH>
Wilking B.</TH><TH>
Univ. of Missouri-St. Louis, MO </TH><TH>
The Nature of Weak Radio Sources in the Rho Oph Cloud Core </TH><TR><TH>
Williams P.</TH><TH>
Royal Observatories - Edinburgh </TH><TH>
Structure of Wolf-Rayet Stellar Winds </TH><TR><TH>
Willis A.</TH><TH>
University College London </TH><TH>
IR Spectroscopy of Wolf-Rayet Starburst Galaxies </TH><TR><TH>
Willis A.</TH><TH>
University College London </TH><TH>
The Neon + Magnesium Abundances in Wc and Wo Stars </TH><TR><TH>
Willner S.</TH><TH>
Smithsonian Astrophysical Observatory - Cambridge </TH><TH>
Abundance Gradient in M 33 </TH><TR><TH>
Winkler C.</TH><TH>
ESA SSD, Noordwijk </TH><TH>
The Infrared Counterpart of Grs 1915+105 Observations of the Quiescent Source</TH><TR><TH>
Winkler C.</TH><TH>
ESA SSD, Noordwijk </TH><TH>
TOO: The Infrared Counterpart of Grs 1915+105 Observations of Outbursts</TH><TR><TH>
Wolstencroft R.</TH><TH>
Royal Observatory, Edinburgh</TH><TH>
Chemistry and Mass-Loss History of a Luminous Carbon Star: IRAS 15194-5115</TH><TR><TH>
Wooden D.</TH><TH>
NASA/AMES Research Center, CA </TH><TH>
Iron-Group Spectroscopy of SN 1987a </TH><TR><TH>
Wouterloot J.</TH><TH>
I. Physikalisches Institut, University of Koeln</TH><TH>
Narrow-Line CO Emission From a Molecular Cloud with Star Formation </TH><TR><TH>
Wozniak H.</TH><TH>
Geneva Observatory - Sauverny </TH><TH>
High Resolution Imaging of (Circum-)Nuclear Starburst Galaxies </TH><TR><TH>
Wright C.</TH><TH>
Max-Planck-Institut fuer extraterrestrische Physik - Garching </TH><TH>
Mid and Far-Infrared Polarimetry of Young Stellar Objects </TH><TR><TH>
Wright C.</TH><TH>
Max-Planck Institut fuer extraterrestrische Physik - Garching </TH><TH>
Formation of Molecular Ice Mantles On Interstellar Dust Grains
And the Nature of the Grain Surfaces.</TH><TR><TH>
Wright G.</TH><TH>
United Kingdom Infrared Telescope, ROE - Edinburgh </TH><TH>
Dust Absorption Features in Active Galaxies </TH><TR><TH>
Xu C.</TH><TH>
MPIK, Heidelberg </TH><TH>
Mapping IR Enhancements in Closely Interacting Spiral-Spiral Pairs </TH><TR><TH>
Xu C.</TH><TH>
MPIK, Heidelberg </TH><TH>
Mapping Intergalactic Dust Emission Compact Groups with Diffuse X-Ray Emission</TH><TR><TH>
Xu C.</TH><TH>
MPIK, Heidelberg </TH><TH>
Mapping the Radio/FIR Ratio Within Five Virgo Galaxies to Study
Disk-ICM Interaction</TH><TR><TH>
Yamamura I.</TH><TH>
Department of Astronomy, University of Tokyo </TH><TH>
Spectroscopic Observations of High-Velocity Flow of Evolved Objects </TH><TR><TH>
Yates J.</TH><TH>
School of Chemistry, University of Bristol </TH><TH>
Observations of FIR Water Masers in Star-Forming Regions. </TH><TR><TH>
Young E.</TH><TH>
University of Arizona, Tucson </TH><TH>
Spectral Energy Distributions in NGC 2264: </TH><TR><TH>
</TH><TH> </TH><TH>A Study of Disk Frequency in a Young Cluster</TH><TR><TH>
Yun M.</TH><TH>
California Institute of Technology - Pasadena </TH><TH>
Star Formation in Young IR Luminous Galaxies </TH><TR><TH>
Zavagno A.</TH><TH>
Observatoire de Marseille and IFSI-CNR - Frascati </TH><TH>
Dust Distribution in Galactic HII Regions </TH><TR><TH>
Zhang C.</TH><TH>
Space Telescope Science Institute </TH><TH>
Spectroscopy of Dusty Planetary Nebulae </TH><TR><TH>
Zijlstra A.</TH><TH>
European Southern Observatory </TH><TH>
Spectroscopy of Planetary Nebulae in the LMC </TH><TR><TH>
Zimmermann T.</TH><TH>
I. Physikalisches Institut Universitaet Zu Koeln </TH><TH>
Molecular-Neutral-Ionized Gas Interfaces in L1457
Line Observations of OI (63 Micron) and CII (158 Micron)</TH><TR><TH>
Zinnecker H.</TH><TH>
Astron. Inst. Univ. Wuerzburg </TH><TH>
Are X-Ray Selected Very Young Weak-Line T Tauri Stars Born Naked? </TH><TR><TH>
Zinnecker H.</TH><TH>
Astron. Inst. Univ. Wuerzburg </TH><TH>
Brown Dwarfs: A Search for Cool Infrared Companions Around Nearby Old
White Dwarfs</TH><TR><TH>
Zinnecker H.</TH><TH>
Astron. Inst. Univ. Wuerzburg </TH><TH>
Remnant Dusty Disks in Lindroos Post T Tauri Stars </TH><TR><TH>
Zuckerman B.</TH><TH>
UCLA - Los Angeles </TH><TH>
Luminosity Class III Stars With Excess Far-IR Emission </TH>
</TABLE>