Towards Population III: The Collapse and Fragmentation of Primordial Gas
Astrophysics
2007-05-23 v1
Abstract
We briefly review the motivations for studying the formation of the first ``Population III'' stars and present recent results from our numerical simulations in this area. We discuss the new questions raised as a result of the simulations presented by us and others at this meeting.
Cite
@article{arxiv.astro-ph/0103382,
title = {Towards Population III: The Collapse and Fragmentation of Primordial Gas},
author = {P. S. Coppi and V. Bromm and R. B. Larson},
journal= {arXiv preprint arXiv:astro-ph/0103382},
year = {2007}
}
Comments
Invited contribution to the proceedings of "The Physics of Galaxy Formation, Tsukuba 2000," in press. 11 pages, 8 postscript figures