Grids of stellar models with rotation I. Models from 0.8 to 120 M ⊙ at solar metallicity (Z = 0.014)

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Ekstrom S ^a   Georgy, C ^b   Eggenberger, P ^a   Meynet, G ^a   Mowlavi, N ^a   Wyttenbach, A ^a   Granada, A ^a,c   Decressin, T ^a   Hirschi, R ^d,e   Frischknecht, U ^d,f   Charbonnel, C ^a,g   Maeder, A ^a  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b UNIVERSITÉ DE LYON   (France)

^c INSTITUTO DE ASTROFÍSICA DE LA PLATA   (Argentina)

^d KEELE UNIVERSITY   (United Kingdom)

^e UNIVERSITY OF TOKYO   (Japan)

^f UNIVERSITY OF BASEL   (Switzerland)

^g UNIVERSITÉ DE TOULOUSE   (France)

Author keywords

Stars: evolution; Stars: general; Stars: low mass; Stars: massive; Stars: rotation

Indexed keywords

STARS: EVOLUTION; STARS: GENERAL; STARS: LOW-MASS; STARS: MASSIVE; STARS: ROTATION;

ASTROPHYSICS; GAMMA RAYS; HELIUM; HYDROGEN; REACTION RATES; ROTATION;

STARS;

EID: 84855957860     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117751     Document Type: Article

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