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Infrared spectroscopy with the Infrared Space Observatory

Published online by Cambridge University Press:  25 May 2016

R. Genzel ,
S. Drapatz ,
D. Lutz ,
C. Wright  and
Th. De Graauw
R. Genzel
Affiliation:
Max-Planck Institut fuer Extraterrestrische Physik, Postfach, 1603, D-85740 Garching, Germany
S. Drapatz
Affiliation:
Max-Planck Institut fuer Extraterrestrische Physik, Postfach, 1603, D-85740 Garching, Germany
D. Lutz
Affiliation:
Max-Planck Institut fuer Extraterrestrische Physik, Postfach, 1603, D-85740 Garching, Germany
C. Wright
Affiliation:
Max-Planck Institut fuer Extraterrestrische Physik, Postfach, 1603, D-85740 Garching, Germany
Th. De Graauw
Affiliation:
Space Research Organization of the Netherlands, P.O. Box 800, 9700 AV Groningen, The Netherlands

Abstract

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The Infrared Space Observatory (ISO) is opening the 2.5 to 200 μm band for detailed infrared spectroscopy. Concentrating on ionic and molecular emission lines observed with the Short Wavelength Spectrometer (SWS) we discuss ISO's first results on Galactic and extragalactic sources.

Type
ISO First Results
Information
Symposium - International Astronomical Union , Volume 178: Molecules in Astrophysics: Probes and Processes , 1997 , pp. 373 - 384
Copyright
Copyright © Kluwer 1997 

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