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On the Extreme Positive Feedback Star-forming Mode from Massive and Compact Super Star Clusters

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Published 2005 July 6 © 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Guillermo Tenorio-Tagle et al 2005 ApJ 628 L13 DOI 10.1086/432665

1538-4357/628/1/L13

Abstract

The force of gravity acting within the volume occupied by young, compact, and massive super star clusters is here shown to drive in situ all the matter deposited by winds and supernovae into several generations of star formation. These events are promoted by radiative cooling, which drains the thermal energy of the ejected gas causing its accumulation to then rapidly exceed the gravitational instability criterion. A detailed account of the integrated ionizing radiation and mechanical luminosity as a function of time is here shown to lead to a new stationary solution. In this, the mass deposition rate , instead of causing a wind as in the adiabatic solution, turns into a positive feedback star-forming mode equal to the star formation rate. Some of the implications of this extreme positive feedback mode are discussed.

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10.1086/432665