CaltechAUTHORS
Published February 1995 | Version public
Journal Article Metadata-only

Chemical Evolution of Circumstellar Matter around Young Stellar Objects

Creators

  • 1. ROR icon Leiden University
  • 2. ROR icon California Institute of Technology

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

Identifiers

Eprint ID
34213
Resolver ID
CaltechAUTHORS:20120919-115758959

Related works

Describes
http://adsabs.harvard.edu/abs/1995Ap%26SS.224..237V (URL)
https://resolver.caltech.edu/CaltechAUTHORS:20200512-142006311 (URL)

Funding

Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
NASA
NAGW-2297
David and Lucille Packard Foundation

Dates

Created
2012-09-19
Created from EPrint's datestamp field
Updated
2021-11-09
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)