Synthetic photometry of globular clusters

Abstract : Color-magnitude diagrams (CMDs) of globular clusters reveal the presence of multiple sequences likely due to populations of stars with different chemical composition (variations in He, C, N, O, Na, Mg, Al). We present synthetic photometry of the globular cluster NGC 6752 based on isochrones and atmosphere models both consistently taking into account such variations of chemical composition. Theoretical CMDs based on this photometry are compared to observed CMDs. We show that CMDs based on red filters are reasonably well reproduced, while those based on blue filters suffer from a number of shortcomings.
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Communication dans un congrès
Journées annuelles de la SF2A, Jul 2017, Paris, France. pp.57 - 60, 2017
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https://hal.archives-ouvertes.fr/hal-01993793
Contributeur : Fabrice Martins <>
Soumis le : mardi 5 février 2019 - 11:29:06
Dernière modification le : jeudi 7 février 2019 - 17:57:59

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2017sf2a.conf..0057M.pdf
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F. Martins, W. Chantereau, C. Charbonnel. Synthetic photometry of globular clusters. Journées annuelles de la SF2A, Jul 2017, Paris, France. pp.57 - 60, 2017. 〈hal-01993793〉

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