Three-body recombination of hydrogen during primordial star formation

Monthly Notices of the Royal Astronomical Society

Volumn 377, Issue 2, 2007, Pages 705-710

  Flower, D R ^a   Harris, G J ^b  

^a DURHAM UNIVERSITY   (United Kingdom)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Cosmology: miscellaneous; Molecular processes; Stars: formation

Indexed keywords

HYDROGEN; POPULATION DISTRIBUTION; STARS;

BOLTZMANN DISTRIBUTION; COSMOLOGY: MISCELLANEOUS; KINETIC TEMPERATURES; MOLECULAR HYDROGEN; MOLECULAR PROCESS; PER UNIT VOLUME; ROVIBRATIONAL LEVELS; STARS FORMATION; STARS: POPULATION III; THREE-BODY RECOMBINATION;

BOLTZMANN EQUATION;

EID: 34247603967     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11632.x     Document Type: Article

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