Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-10-26
Astrophys.J. 620 (2005) 217-222
Astronomy and Astrophysics
Astrophysics
11 pages, 5 figures, accepted for publication by The Astrophysical Journal
Scientific paper
10.1086/426962
The properties of star cluster winds in the supercritical, catastrophic cooling regime are discussed. We demonstrate that strong radiative cooling may inhibit superwinds and, after a rapid phase of accumulation of the ejected material within the star-forming volume, a new stationary isothermal regime, supported by the ionizing radiation from the central cluster, is established. The expected appearance of this core/halo supernebula in the visible line regime and possible late evolutionary tracks for super-star cluster winds, in the absence of ionizing radiation, are thoroughly discussed.
Munoz-Tunon Casiana
Rodriguez-Gonzalez Ary
Silich Sergiy
Tenorio-Tagle Guillermo
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