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Chemical Evolution of Circumstellar Matter around Young Stellar Objects

van Dishoeck, Ewine F. and Blake, Geoffrey A. (1995) Chemical Evolution of Circumstellar Matter around Young Stellar Objects. Astrophysics and Space Science, 224 (1-2). pp. 237-249. ISSN 0004-640X. doi:10.1007/BF00667852. https://resolver.caltech.edu/CaltechAUTHORS:20120919-115758959

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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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/BF00667852DOIArticle
http://adsabs.harvard.edu/abs/1995Ap%26SS.224..237VADSArticle
https://resolver.caltech.edu/CaltechAUTHORS:20200512-142006311Related ItemConference Paper
ORCID:
AuthorORCID
van Dishoeck, Ewine F.0000-0001-7591-1907
Blake, Geoffrey A.0000-0003-0787-1610
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.
Funders:
Funding AgencyGrant Number
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)UNSPECIFIED
NASANAGW-2297
David and Lucille Packard FoundationUNSPECIFIED
Subject Keywords:Molecular abundances; young stellar objects; (sub)millimeter observations
Issue or Number:1-2
DOI:10.1007/BF00667852
Record Number:CaltechAUTHORS:20120919-115758959
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20120919-115758959
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34213
Collection:CaltechAUTHORS
Deposited By:INVALID USER
Deposited On:19 Sep 2012 22:05
Last Modified:09 Nov 2021 23:07

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