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Chemical Characteristics of Embedded Young Stellar Objects

Published online by Cambridge University Press:  25 May 2016

Michiel R. Hogerheijde*
Affiliation:
Astronomy Department, 601 Campbell Hall, University of California, Berkeley, CA 94720-3411, USA

Abstract

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Based on theoretical considerations, the chemistry around embedded young stellar objects is expected to be governed by the interplay between gas-phase reactions, condensation of molecules onto dust grains, grain surface reactions, and evaporation of altered ice mantles near the star and in the outflow. I discuss the chemical characteristics of embedded young stellar objects, with special emphasis on these processes.

Type
Part 1. Chemistry in Pre-Stellar Cores and Low-Mass Star-Forming Regions
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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