Winds Driven by Super-Star Clusters

Bibcode
2004RMxAC..22..152S
Silich, S.; Tenorio-Tagle, G.; Rodríguez-González, A.; Muñoz-Tuñon, C.
Bibliographical reference

Gravitational Collapse: From Massive Stars to Planets. / First Astrophysics meeting of the Observatorio Astronomico Nacional. / A meeting to celebrate Peter Bodenheimer for his outstanding contributions to Astrophysics. (Eds. G. García-Segura, G. Tenorio-Tagle, J. Franco, & H. W. Yorke) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 22, pp. 152-155 (2004) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
12
2004
Number of authors
4
IAC number of authors
0
Citations
0
Refereed citations
0
Description
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 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. Finally, we discuss the expected appearance of the supergalactic winds driven by multiple super-star clusters.
Type
Non-refereed
Galaxies
Star clusters

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