The atomic-to-molecular transition in galaxies. III. A new method for determining the molecular content of primordial and dusty clouds

Astrophysical Journal

Volumn 709, Issue 1, 2010, Pages 308-320

  McKee, Christopher F ^a   Krumholz, Mark R ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

ISM: clouds; ISM: molecules; Molecular processes; Radiative transfer; Stars: formation

Indexed keywords

EID: 73849143847     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/709/1/308     Document Type: Article

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