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2022MNRAS.509.4208V - Mon. Not. R. Astron. Soc., 509, 4208-4228 (2022/January-3)
Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si. II. Application to the colour-magnitude diagrams of the globular clusters 47 Tuc, NGC 6362, M 5, M 3, M 55, and M92.
VANDENBERG D.A., CASAGRANDE L. and EDVARDSSON B.
Abstract (from CDS):
Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
Journal keyword(s): stars: abundances - stars: evolution - Hertzsprung-Russell and colour-magnitude diagrams - stars: Population II - globular clusters: general
Simbad objects: 16
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