Fragmentation of the Primordial Gas Clouds and the Lower Limit on the Mass of the First Stars
نویسندگان
چکیده
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. Subject headings: galaxies: formation—molecular processes— stars: formation
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تاریخ انتشار 1996