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Astron. Astrophys. 315, L357-L360 (1996)

An ISO SWS view of interstellar ices: first results*

D.C.B. Whittet1, W.A. Schutte2, A.G.G.M. Tielens3, A.C.A. Boogert4, Th.de Graauw4, P.Ehrenfreund2, P.A. Gerakines1, F.P. Helmich2, T. Prusti5, and E.F. van Dishoeck2

1 Department of Physics, Applied Physics & Astronomy, Rensselaer Polytechnic Institute, Troy, NY 12180, USA
2 Leiden Observatory, P.O. Box 9513, 2300 RA Leiden, The Netherlands
3 NASA Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035, USA
4 SRON, PO Box 800, 9700 AV Groningen, The Netherlands
5 ISO Science Operations Centre, Astrophysics Division, ESA, Villafranca del Castillo, P.O. Box 50727, E-28080 Madrid, Spain

Received 18 July 1996 / Accepted 23 August 1996

Abstract. The availability of SWS data from the Infrared Space Observatory is a landmark in the study of interstellar ices. This paper presents a brief review of what was known prior to the launch of ISO, and attempts a synthesis of what has been learned from the ISO observations available to date. Key areas of uncertainty are identified to provide a basis for future research.

Key words: ISM: molecules - dust, extinction - infrared: interstellar: lines - stars: pre-main sequence

* Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries France, Germany, the Netherlands and the United Kingdom) and with the participation of ISAS and NASA.

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Last change: December 16, 1996
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