The relationship between the WR classification and stellar models II. The WN stars without hydrogen

Astronomy and Astrophysics

Volumn 334, Issue 3, 1998, Pages 845-856

  Smith, Lindsey F ^a   Maeder, A ^b  

^a UNIVERSITY OF SYDNEY   (Australia)

^b UNIVERSITÉ DE GENÈVE   (Switzerland)

Author keywords

Abundances; Stars: evolution; Wolf Rayet

Indexed keywords

EID: 0000522775     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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