Line intensities for CH and their application to stellar atmospheres

Astronomy and Astrophysics

Volumn 315, Issue 1, 1996, Pages 204-211

  Jorgensen U G ^a   Larsson, M ^b   Iwamae, A ^b,c   Yu, B ^b  

^a UNIVERSITY OF COPENHAGEN   (Denmark)

^b ROYAL INSTITUTE OF TECHNOLOGY   (Sweden)

^c KYOTO UNIVERSITY   (Japan)

Author keywords

Molecular data; Stars: atmospheres; Stars: carbon

Indexed keywords

EID: 0043257577     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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