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Star cluster winds: The impact of radiative cooling

Published online by Cambridge University Press:  24 November 2004

Sergiy Silich ,
G. Tenorio-Tagle  and
A. Rodríguez-González
Sergiy Silich
Affiliation:
Instituto Nacional de Astrofísica Optica y Electrónica, AP 51, 72000 Puebla, Mexico email: [email protected]
G. Tenorio-Tagle
Affiliation:
Instituto Nacional de Astrofísica Optica y Electrónica, AP 51, 72000 Puebla, Mexico email: [email protected]
A. Rodríguez-González
Affiliation:
Instituto Nacional de Astrofísica Optica y Electrónica, AP 51, 72000 Puebla, Mexico email: [email protected]
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Abstract

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Here we present a self-consistent stationary solution for spherically symmetric winds driven by massive star clusters under the impact of radiative cooling. We demonstrate that cooling may modify drastically the distribution of temperature and the observational appearance of star cluster winds if the rate of injected energy approaches a critical value, and that the stationary wind solution does not exist if the energy deposition rate exceeds this limit.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 213 - 214
Copyright
© 2004 International Astronomical Union