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Models and Observations of the Chemistry Near Young Stellar Objects

  • Chapter
The Origin of Stars and Planetary Systems

Part of the book series: NATO Science Series ((ASIC,volume 540))

Abstract

The study of the chemical evolution of gas and dust from pre-stellar dense cores to circumstellar disks around young stars forms an essential part of understanding star- and planet formation. Throughout the collapse- and protostellar phases, simple and complex molecules are formed, many of which deplete onto cold grains and are eventually incorporated into the icy planetesimals of new solar systems (see Figure 1). Tracing this chemical evolution provides a wealth of information, not only about the chemical processing in primitive solar nebulae, but also about physical processes which occur in the immediate surroundings of young stellar objects (YSOs).

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Authors and Affiliations

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

    Ewine F. Van Dishoeck

  2. Astronomy Department, Univ. of California, Berkeley, CA, 94720, USA

    Michiel R. Hogerheijde

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  1. Ewine F. Van Dishoeck
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  1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA

    Charles J. Lada

  2. Department of Physics, University of Crete, Heraklion, Crete, Greece

    Nikolaos D. Kylafis

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Van Dishoeck, E.F., Hogerheijde, M.R. (1999). Models and Observations of the Chemistry Near Young Stellar Objects. In: Lada, C.J., Kylafis, N.D. (eds) The Origin of Stars and Planetary Systems. NATO Science Series, vol 540. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4509-1_4

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