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Chemical Evolution of Circumstellar Matter around Young Stellar Objects

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Circumstellar Matter 1994

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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.

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Author information

Authors and Affiliations

  1. Leiden Observatory, P.O. Box 9513, 2300 RA, Leiden, The Netherlands

    Ewine F. van Dishoeck

  2. California Institute of Technology, 170-25 Pasadena, CA, 91125, USA

    Geoffrey A. Blake

Authors
  1. Ewine F. van Dishoeck
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  2. Geoffrey A. Blake
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Editor information

G. D. Watt P. M. Williams

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© 1995 Springer Science+Business Media Dordrecht

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van Dishoeck, E.F., Blake, G.A. (1995). Chemical Evolution of Circumstellar Matter around Young Stellar Objects. In: Watt, G.D., Williams, P.M. (eds) Circumstellar Matter 1994. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0147-9_41

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  • DOI: https://doi.org/10.1007/978-94-011-0147-9_41

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4066-2

  • Online ISBN: 978-94-011-0147-9

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