On the Extreme Stationary Outflows from Super Star Clusters: From Superwinds to Supernebulae and Further Massive Star Formation

Bibcode
2005ApJ...620..217T
DOI
10.1086/426962
Tenorio-Tagle, Guillermo; Silich, Sergiy; Rodríguez-González, Ary; Muñoz-Tuñón, Casiana
Bibliographical reference

The Astrophysical Journal, Volume 620, Issue 1, pp. 217-222.

Advertised on:
2
2005
Journal
The Astrophysical Journal
Number of authors
4
IAC number of authors
1
Citations
25
Refereed citations
18
Description
Here we discuss the properties of star cluster winds in the supercritical, catastrophic cooling regime. We demonstrate that catastrophic cooling inhibits superwinds and that 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 of super star cluster winds in the absence of ionizing radiation are thoroughly discussed.
Type
Refereed
Galaxies
Methods

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