A rotational-level hydrogen physical chemistry model for general astrophysical application

Astrophysical Journal

Volumn 624, Issue 1 I, 2005, Pages 448-461

  Hallett, J T ^a   Shemansky, D E ^a   Liu, X ^a  

^a University of Southern California ^*  (United States)

Author keywords

Atomic processes; Comets: general; Diffusion; Molecular processes; Planets and satellites: general; Stars: atmospheres

Indexed keywords

EID: 20344397723     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/428935     Document Type: Article

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