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Photodissociative Regulation of Star Formation in Metal‐free Pregalactic Clouds
Author(s) -
Kazuyuki Omukai,
Ryoichi Nishi
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/307285
Subject(s) - stars , star formation , astrophysics , reionization , physics , molecular cloud , protostar , universe , astronomy , photodissociation , star (game theory) , galaxy , chemistry , redshift , photochemistry
We study the H2 photodissociation regions around OB stars in primordial gasclouds whose virial temperatures are between a few hundred and a few thousandKelvin. In such small objects, a single O star can photodissociate a mass equalto that of the cloud itself. As a result, the clouds deplete their molecularcoolant and cannot cool in a free-fall time, and subsequent star formation istotally quenched. This indicates that stars do not form efficiently in smallobjects and that these objects contribute little to the reionization of theuniverse.Comment: 9 pages. ApJ, 518, in pres

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