Published 1995
| public
Book Section - Chapter
Chemical Evolution of Circumstellar Matter around Young Stellar Objects
- Creators
-
van Dishoeck, Ewine F.
-
Blake, Geoffrey A.
- Others:
- Watt, G. D.
- Williams, P. M.
Chicago
An error occurred while generating the citation.
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. 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
- 103152
- Resolver ID
- CaltechAUTHORS:20200512-142006311
- Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
- NASA
- NAGW-2297
- David and Lucille Packard Foundation
- Created
-
2020-05-12Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)