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Models of hot molecular cores

Published online by Cambridge University Press:  25 May 2016

T.J. Millar
T.J. Millar*
Affiliation:
Department of Physics, UMIST, P.O. Box 88, Manchester M60 1QD, England

Abstract

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We review the properties of hot molecular cores with specific reference to chemical modelling. While most theoretical modelling has been generic, we discuss models for two specific sources, G34.3+0.15 and W3 (H2O). We show that the hot core gas in both these regions has an age of 5 103 — 104 yrs and that the abundances of many molecules are consistent with formation in the gas-phase following evaporation of simple molecular ices from the grains. We end with a discussion of current problems and future directions.

Type
Star Formation
Information
Symposium - International Astronomical Union , Volume 178: Molecules in Astrophysics: Probes and Processes , 1997 , pp. 75 - 88
Copyright
Copyright © Kluwer 1997 

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