Experimental results for H2 formation from H-and H and implications for first star formation

Science

Volumn 329, Issue 5987, 2010, Pages 69-71

  Kreckel, H ^a,e   Bruhns, H ^a,f   Cizek M ^b   Glover, S C O ^c   Miller, K A ^a   Urbain, X ^d   Savin, D W ^a  

^a Och Spine at New York Presbyterian Hospitals   (United States)

^b CHARLES UNIVERSITY   (Czech Republic)

^c UNIVERSITY OF HEIDELBERG   (Germany)

^d UNIVERSITÉ CATHOLIQUE DE LOUVAIN   (Belgium)

^e UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^f INFICON GmbH   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

HYDROGEN;

COSMOLOGY; CROSS SECTION; GAS FLOW; HYDROGEN; NUMERICAL MODEL; TEMPERATURE EFFECT; THEORETICAL STUDY; UNCERTAINTY ANALYSIS;

ARTICLE; ASTRONOMY; COSMOS; ENERGY; GAS; HYDRODYNAMICS; PRIORITY JOURNAL; SIMULATION; STATIC ELECTRICITY; TEMPERATURE; THEORETICAL MODEL; TIME;

EID: 77954328999     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1187191     Document Type: Article

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28. Supported by the Deutscher Akademischer Austauschdienst (H.B.); Grantová Agentura České Republiky grant 202/07/ 0833 and "Výzkumný záměr" grant MSM 0021620860 (M.C.̌.); German Bundesministerium für Bildung und Forschung (via STAR FORMAT grant 05A09VHA), Deutsche Forschungsgemeinschaft grant KL1358/4, and Heidelberg University, sponsored by the German Excellence Initiative and the Landesstiftung Baden-Württemberg (International Collaboration Il grant P-LS-SPII/18) (S.C.O.G.); and NSF grants CHE-0520660, AST-0606960, and AST-0807436. X.U. is a Senior Research Associate of the Fonds de la Recherche Scientifique-FNRS, Belgium.