On The use of the self-consistent-field method in the construction of models for rapidly rotating main-sequence stars

Astrophysical Journal, Supplement Series

Volumn 156, Issue 2, 2005, Pages 245-264

  Jackson, Stephen ^a   Macgregor, Keith B ^a   Skumanich, Andrew ^a  

^a NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

Methods: numerical; Stars: interiors; Stars: rotation

Indexed keywords

EID: 14644406753     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/426587     Document Type: Article

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