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ISO Results on Star Formation and Early Stellar Evolution

Published online by Cambridge University Press:  14 August 2015

Thierry Montmerle  and
Lennart Nordh
Thierry Montmerle
Affiliation:
Service d'Astrophysique CEA/DSM/DAPNIA/SAp, Centre d'Etudes de SaclayF-91191 Gif-sur-Yvette Cedex, France
Lennart Nordh
Affiliation:
Stockholm ObservatoryS-13336 Saltsjöbaden, Sweden

Extract

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With all its instruments, ISO is sensitive to temperatures in the range ~ 30 – 2000 K. This range is particularly adapted to studies of dense interstellar matter (gas and dust) in cold clouds, and to material associated with very early stages of stellar evolution: circumstellar matter around low-mass stars (disks, envelopes), outflows generated by them and interactions with the surrounding medium.

Type
III. Special Scientific Sessions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 1137 - 1139
Copyright
Copyright © Kluwer 1998

References

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