The formation of population III binaries from cosmological initial conditions

Science

Volumn 325, Issue 5940, 2009, Pages 601-605

  Turk, Matthew J ^a   Abel, Tom ^a   O'Shea, Brian ^b  

^a STANFORD UNIVERSITY   (United States)

^b MICHIGAN STATE UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

HYDROGEN;

COOLING; COSMOLOGY; EXTRATERRESTRIAL MATTER; HYDROGEN;

ARTICLE; ASTRONOMY; CONTROLLED STUDY; COOLING; COSMOS; DENSITY; FIELD EMISSION; GAS; MASS; MASS FRAGMENTOGRAPHY; MOLECULE; POPULATION; PREDICTION; PRIORITY JOURNAL; RADIATION; RESERVOIR; SIMULATION; SUN;

EID: 68149105915     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1173540     Document Type: Article

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32. We thank V. Bromm, G. Bryan, A. Escala, S. Glover, C. McKee, J. Oishi, B. Smith, J. Tumlinson, and N. Yoshida for useful discussions. This work was partially supported by the U.S. Department of Energy (DOE) contract to Stanford Linear Accelerator Center no. DE-AC02-76SF00515, NASA Astrophysics Theory and Fundamental Physics grant NNX08AH26G, and NSF AST-0807312. B.W.O. and M.J.T. carried out this work in part under the auspices of the National Nuclear Security Administration of the DOE at Los Alamos National Laboratory (LANL) under contract no. DE-AC52-06NA25396. B.W.O. was partially supported by a LANL Director's Postdoctoral Fellowship (DOE LDRD grant 20051325PRD4).