Forming the First Stars in the Universe: The Fragmentation of Primordial Gas
- 10 December 1999
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 527 (1), L5-L8
- https://doi.org/10.1086/312385
Abstract
In order to constrain the initial mass function of the first generation of stars (Population III), we investigate the fragmentation properties of metal-free gas in the context of a hierarchical model of structure formation. We investigate the evolution of an isolated 3 σ peak of mass 2 × 106 M☉ that collapses at zcoll 30 using smoothed particle hydrodynamics. We find that the gas dissipatively settles into a rotationally supported disk that has a very filamentary morphology. The gas in these filaments is Jeans unstable with MJ ~ 103 M☉. Fragmentation leads to the formation of high-density (n > 108 cm-3) clumps that subsequently grow in mass by accreting the surrounding gas and by merging with other clumps up to masses of ~104 M☉. This suggests that the very first stars were rather massive. We explore the complex dynamics of the merging and tidal disruption of these clumps by following their evolution over a few dynamical times.Keywords
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