Winds Driven by Super-Star Clusters

Details Winds Driven by Super-Star Clusters Winds Driven by Super-Star Clusters

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..22..152s&link_type=abstract

Gravitational Collapse: From Massive Stars to Planets. / First Astrophysics meeting of the Observatorio Astronomico Nacional. /

Astronomy and Astrophysics

Astrophysics

Galaxies: Star Clusters, Stars: Winds, Outflows

Scientific paper

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.

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