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Star – Gas Cycle in Galaxies

Published online by Cambridge University Press:  01 August 2006

Jan Palouš
Jan Palouš*
Affiliation:
Astronomical Institute, Academy of Sciences, Boční II 1401, 140 41 Prague 4, Czech Republic email: palous@ig.cas.cz
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Abstract

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The importance of the star-gas cycle for the evolution of galaxies is discussed. We describe three different ways of stellar mass loss: a) the gas return from low and intermediate mass stars, b) the stellar winds from OB associations; c) the superwinds from superstar clusters.

Keywords

supernovae: generalstars: windsISM: abundancesISM: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 268 - 270
Copyright
Copyright © International Astronomical Union 2007

References

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