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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

Bournaud, F., Combes, F. & Semelin, B. 2005 MNRAS 364, 18.CrossRefGoogle Scholar
Brüns, C., Kerp, J., Staveley-Smith, L. 2004 A&A 432, 45.Google Scholar
de Grijs, R., O'Connell, R. W. & Gallagher, J. S. 2001 ApSS 276, 397.Google Scholar
Efremov, Yu. N., Ehlerová, S. & Palouš, J. 1999 A&A 350, 457.Google Scholar
Jungwiert, B. 2006 this volume.Google Scholar
Jungwiert, B., Combes, F. & Palouš, J. 2001 A&A 376, 85.Google Scholar
van der Hulst, T. & Sancisi, R. 2004 IAU Symp. 217, 122.Google Scholar
Tenorio-Tagle, G., Wünsch, R., Silich, S. & Palouš, J. 2006 ApJ submitted.Google Scholar
Zhang, Q., Fall, S. M. & Whitmore, B. C 2001 ApJ 561, 727.CrossRefGoogle Scholar