Breathing in Low-Mass Galaxies: A Study of Episodic Star Formation

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© 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation G. S. Stinson et al 2007 ApJ 667 170 DOI 10.1086/520504

0004-637X/667/1/170

Abstract

We simulate the collapse of isolated dwarf galaxies using SPH + N-body simulations including a physically motivated description of the effects of supernova feedback. As the gas collapses and stars form, the supernova feedback disrupts enough gas to temporarily quench star formation. The gas flows outward into a hot halo, where it cools until star formation can continue once more and the cycle repeats. The star formation histories of isolated Local Group dwarf galaxies exhibit similar episodic bursts of star formation. We examine the mass dependence of the stellar velocity dispersions and find that they are no less than half the velocity of the halos measured at the virial radius.

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10.1086/520504