The transition from atomic to molecular hydrogen in interstellar clouds: 21 cm signature of the evolution of cold atomic hydrogen in dense clouds

Astrophysical Journal

Volumn 654, Issue 1 I, 2007, Pages 273-289

  Goldsmith, Paul F ^a   Li, Di ^a   Krčo, Marko ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b Department of Population Medicine and Diagnostic Sciences   (United States)

Author keywords

ISM: atoms; ISM: evolution; ISM: individual (hydrogen); ISM: molecules

Indexed keywords

EID: 33846539777     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/509067     Document Type: Article

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