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Submillimetre Observations of UC HII Regions and Hot Molecular Cores

Published online by Cambridge University Press:  25 May 2016

G. H. Macdonald  and
M. A. Thompson
G. H. Macdonald
Affiliation:
Electronics Laboratory, University of Kent, Canterbury, Kent, UK
M. A. Thompson
Affiliation:
Electronics Laboratory, University of Kent, Canterbury, Kent, UK

Abstract

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Recent submillimetre observations of continuum radiation from warm dust and molecular line emission from hot gas in regions of high mass star formation are reviewed. Such regions are characterised by ultracompact HII regions around young OB stars and associated hot molecular cores which appear to harbour high mass protostars at an earlier stage of evolution.

Type
Part 2. Chemistry in High-Mass Star-Forming Regions
Information
Symposium - International Astronomical Union , Volume 197: Astrochemistry: From Molecular Clouds to Planetary Systems , 2000 , pp. 113 - 124
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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