Stellar models with the ML2 theory of convection

Astronomy and Astrophysics

Volumn 487, Issue 3, 2008, Pages 1075-1080

  Salaris, M ^a   Cassisi, S ^b  

^a LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^b INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

Author keywords

Convection; Globular clusters: general; Stars: evolution; Stars: interiors; Sun: general; Turbulence

Indexed keywords

ASTRONOMY; BOUNDARY LAYERS; CHLORINE COMPOUNDS; EARTH ATMOSPHERE; KETONES; MIXING; STANDARDS; STARS;

A-PRIORI; CONVECTION; CRUDE APPROXIMATIONS; FREE PARAMETERS; GALACTIC GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: GENERAL; MIXING LENGTH; MODEL ATMOSPHERE; MODEL COMPUTATIONS; RED GIANTS; SOLAR MODELING; STANDARD FORM; STARS: EVOLUTION; STARS: INTERIORS; STELLAR EVOLUTIONS; STELLAR INTERIOR; STELLAR MODELING; SUN: GENERAL; TEMPERATURE GRADIENTS; THREE PARAMETERS; TURBULENCE; WHITE DWARF;

PETROLEUM ENGINEERING;

EID: 49749102012     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810253     Document Type: Article

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