Stellar evolution models for Z = 0.0001 to 0.03

Monthly Notices of the Royal Astronomical Society

Volumn 298, Issue 2, 1998, Pages 525-536

  Pols, Onno R ^a,b   Schröder, Klaus Peter ^b,c   Hurley, Jarrod R ^b   Tout, Christopher A ^b   Eggleton, Peter P ^b  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c Inst F Astronomie und Astrophysik   (Germany)

Author keywords

Convection; Galaxies: stellar content; Hertzsprung Russell (HR) diagram; Open clusters and associations: general; Stars: evolution; Stars: Population II

Indexed keywords

HELIUM; MIXING; STARS;

CONVECTION; GALAXY:STELLAR CONTENT; HERTZSPRUNG-RUSSELL DIAGRAMS; ISOCHRONES; METALLICITIES; OPEN CLUSTERS; OPEN CLUSTERS AND ASSOCIATIONS: GENERAL; STAR: EVOLUTION; STARS: POPULATION II; STELLAR EVOLUTIONS;

ASTROPHYSICS;

EID: 0000247257     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01658.x     Document Type: Article

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