Published February 1995
| public
Journal Article
Chemical Evolution of Circumstellar Matter around Young Stellar Objects
- Creators
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van Dishoeck, Ewine F.
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Blake, Geoffrey A.
Chicago
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Abstract
Recent observational studies of the chemical composition of circumstellar matter around both high- and low-mass young stellar objects are reviewed. The molecular abundances are found to be a strong function of evolutionary state, but not of system mass or luminosity. The data are discussed with reference to recent theoretical models.
Additional Information
© 1995 Kluwer Academic Publishers. Publication date: February 1995. This work was supported by a PIONIER grant from the Netherlands Organization of Scientific Research (NWO), and by NASA grant NAGW-2297 as well as the David and Lucille Packard Foundation.Additional details
- Eprint ID
- 34213
- Resolver ID
- CaltechAUTHORS:20120919-115758959
- Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
- NASA
- NAGW-2297
- David and Lucille Packard Foundation
- Created
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2012-09-19Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)