EFFECTS OF VARYING THE THREE-BODY MOLECULAR HYDROGEN FORMATION RATE IN PRIMORDIAL STAR FORMATION-Reference-Cited by-同舟云学术

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EFFECTS OF VARYING THE THREE-BODY MOLECULAR HYDROGEN FORMATION RATE IN PRIMORDIAL STAR FORMATION

Published:2010-12-14 Issue:1 Volume:726 Page:55
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Turk Matthew J.,Clark Paul,Glover S. C. O.,Greif T. H.,Abel Tom,Klessen Ralf,Bromm Volker

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/726/i=1/a=55/pdf

Reference44 articles.

1. The Formation of the First Star in the Universe

2. Smooth Particle Hydrodynamics: A Review

3. The Formation of the First Stars. I. The Primordial Star‐forming Cloud

4. The First Stars

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