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

Citation

VandenBerg, D, Casagrande, L & Edvardsson, B 2022, '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', Monthly Notices of the Royal Astronomical Society, vol. 509, no. 3, pp. 4208-4228.

Year

2022

ANU Authors

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