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Volumn 12, Issue 2, 2003, Pages 247-251
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The consequences of assuming m=0 for global model-fitting
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Author keywords
Methods: Numerical stars: Individual (GD 358); Stars: White dwarfs; Stars:Oscillations
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Indexed keywords
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EID: 2542631759
PISSN: 13920049
EISSN: None
Source Type: Journal
DOI: 10.1515/astro-2017-0048 Document Type: Article |
Times cited : (11)
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References (7)
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