Winds Driven by Super-Star Clusters

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

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/)

Fecha de publicación:
12
2004
Número de autores
4
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro
Galaxias
Cúmulos de estrellas

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