Non-gray rotating stellar models and the evolutionary history of the Orion Nebular Cluster

Astronomy and Astrophysics

Volumn 456, Issue 1, 2006, Pages 269-282

  Landin, N R ^a,b   Ventura, P ^b   D'Antona, F ^b   Mendes, L T S ^a   Vaz, L P R ^a  

^a FEDERAL UNIVERSITY OF MINAS GERAIS   (Brazil)

^b INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

Author keywords

Stars: evolution; Stars: Hertzsprung Russell (HR) and C M diagrams; Stars: interiors; Stars: rotation

Indexed keywords

BOUNDARY CONDITIONS; CALIBRATION; COMPUTER SIMULATION; HEAT CONVECTION; HYDRODYNAMICS; MAGNETIC FIELD EFFECTS; MATHEMATICAL MODELS; ROTATION;

STARS: EVOLUTION; STARS: HERTZSPRUNG-RUSSELL (HR) AND C-M DIAGRAMS; STARS: INTERIORS; STARS: ROTATION;

ASTROPHYSICS;

EID: 33748687173     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054011     Document Type: Article

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