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HI and HII in Nearby Spiral Galaxies

Published online by Cambridge University Press:  03 August 2017

F. Viallefond
F. Viallefond*
Affiliation:
Department of Millimeter Radioastronomy, Observatoire de Meudon, F92190 FRANCE

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Spiral arm properties varies widely from one galaxy to another. For this reason detailed observational studies of galaxies with different morphologies are critical for the understanding of the role, if any, of the spiral arms, in the formation of the complexes of HI clouds, molecular clouds and ultimately for the formation of the massive stars.

Type
VI- Other Gaseous Components
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 167 - 179
Copyright
Copyright © Kluwer 1991 

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