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Volumn 392, Issue 1, 2002, Pages 115-129
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Does the mixing length parameter depend on metallicity? Further tests of evolutionary sequences using homogeneous databases
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Author keywords
Galaxy: globular clusters: general; Galaxy: halo; Stars: evolution; Stars: Hertzsprung Russell (HR) and C M diagrams; Stars: horizontal branch; Stars: population II
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Indexed keywords
ASTROPHYSICS;
ATMOSPHERIC TEMPERATURE;
CALIBRATION;
COLOR;
COMPUTER SIMULATION;
DATABASE SYSTEMS;
IRON;
PHOTOMETRY;
GLOBULAR CLUSTERS;
HALO;
METALLICITY;
MIXING LENGTH PARAMETER;
STARS;
GALAXIES;
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EID: 0036733969
PISSN: 00046361
EISSN: None
Source Type: Journal
DOI: 10.1051/0004-6361:20020840 Document Type: Article |
Times cited : (23)
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References (41)
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