New grids of stellar models including tidal-evolution constants up to carbon burning II. From 0.8 to 125 Mo: The Small Magellanic Cloud (Z=0.002-0.004)

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[1] Claret, A.

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Claret, A. (claret@iaa.es) | 1600年 / EDP Sciences卷 / 440期

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[1] New grids of stellar models including tidal-evolution constants up to carbon burning -: II.: From 0.8 to 125 M⊙ :: the Small Magellanic Cloud (Z=0.002-0.004)
Claret, A
ASTRONOMY & ASTROPHYSICS, 2005, 440 (02) : 647 - 651
[2] New grids of stellar models including tidal-evolution constants up to carbon burning III.: From 0.8 to 125 M⊙:: the Large Magellanic Cloud (Z=0.007-0.01)
Claret, A.
ASTRONOMY & ASTROPHYSICS, 2006, 453 (02) : 769 - 771
[3] New grids of stellar models including tidal-evolution constants up to carbon burning -: I.: From 0.8 to 125 M⊙ at Z=0.02
Claret, A
ASTRONOMY & ASTROPHYSICS, 2004, 424 (03) : 919 - 925
[4] New grids of stellar models including tidal-evolution constants up to carbon burning IV. From 0.8 to 125 Mo: High metallicities (Z= 0.04-0.10)
Claret, A.
1600, EDP Sciences, 17 Avenue du Hoggar - BP 112, Les Ulis Cedex A, F-91944, France (467):
[5] New grids of stellar models including tidal-evolution constants up to carbon burning -: IV.: From 0.8 to 125 M⊙:: high metallicities (Z=0.04-0.10)
Claret, A.
ASTRONOMY & ASTROPHYSICS, 2007, 467 (03) : 1389 - 1396