Towards Population III: The Collapse and Fragmentation of Primordial Gas

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dc.creatorCoppi, P. S.
dc.creatorBromm, V.
dc.creatorLarson, R. B.
dc.date2001-03-22
dc.date.accessioned2026-07-07T01:57:59Z
dc.date.available2026-07-07T01:57:59Z
dc.descriptionWe 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.
dc.descriptionInvited contribution to the proceedings of "The Physics of Galaxy Formation, Tsukuba 2000," in press. 11 pages, 8 postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0103382
dc.identifierhttp://arxiv.org/abs/astro-ph/0103382
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2602
dc.subjectAstrophysics
dc.titleTowards Population III: The Collapse and Fragmentation of Primordial Gas
dc.typetext

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