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Volumn 675, Issue 1, 2008, Pages 746-763
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On the use of blanketed atmospheres as boundary conditions for stellar evolutionary models
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Author keywords
Globular clusters: individual (M68); Hertzsprung Russell diagram; Open clusters and associations: individual (M67); Stars: atmospheres; Stars: evolution; Stars: fundamental parameters (temperatures); Sun: abundances
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Indexed keywords
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EID: 40249090498
PISSN: 0004637X
EISSN: 15384357
Source Type: Journal
DOI: 10.1086/521600 Document Type: Article |
Times cited : (60)
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References (70)
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