2-D non-LTE models of radiation driven winds from rotating early-type stars: I. Winds with an optically thin continuum

Astronomy and Astrophysics

Volumn 358, Issue 3, 2000, Pages 956-992

  Petrenz, P ^a   Puls, J ^a  

^a UNIVERSITY OF MUNICH   (Germany)

Author keywords

Hydrodynamics; Methods: numerical; Stars: circumstellar matter; Stars: early type; Stars: mass loss; Stars: rotation

Indexed keywords

EID: 0000247486     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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