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The Molecular Cloud Content of Spiral and Dwarf Galaxies

Published online by Cambridge University Press:  30 March 2016

L. J Rickard
L. J Rickard*
Affiliation:
Sachs/Freeman Associates, Inc., and E. O. Hulburt Center for Space Research, Naval Research Laboratory, and Department of Physics and Astronomy, Howard University, U.S.A.

Abstract

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This paper concentrates on the molecular cloud component in its role as the site of current star formation – especially massive star formation. It is further restricted to the molecular component as traced by CO, the preeminent tracer of molecular gas in galaxies despite the problems discussed here. The basic topics addressed are (1) the variation of CO properties with galactic environment and type; (2) the problems involved in the inference of H2 distributions for individual galaxies from CO observations; and (3) the particular question of the presence of spiral structure in the CO component.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 519 - 524
Copyright
Copyright © Reidel 1986

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