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Fragmentation of the Primordial Gas Clouds and the Lower Limit on the Mass of the First Stars

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©1996. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Hideya Uehara et al 1996 ApJ 473 L95 DOI 10.1086/310409

1538-4357/473/2/L95

Abstract

We discuss the fragmentation of primordial gas clouds in the universe after decoupling. Comparing the timescale of collapse with that of fragmentation, we obtain the typical mass of a fragment both numerically and analytically. We show that the estimated mass gives the minimum mass of a fragment that is formed from the primordial gas cloud and essentially determined by the Chandrasekhar mass.

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10.1086/310409