The C+N+O abundance of ω Centauri giant stars: implications for the 
chemical-enrichment scenario and the relative ages of different stellar 
populations

Marino, A. F.; Milone, A. P.; Piotto, G.; Cassisi, S.; D'Antona, F.; Anderson, J.; Aparicio, A.; Bedin, L. R.; Renzini, A.; Villanova, S.

doi:10.1088/0004-637X/746/1/14

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The C+N+O abundance of ω Centauri giant stars: implications for the chemical-enrichment scenario and the relative ages of different stellar populations

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Marino, A. F.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Marino, A. F., Milone, A. P., Piotto, G., Cassisi, S., D'Antona, F., Anderson, J., et al. (2012). The C+N+O abundance of ω Centauri giant stars: implications for the chemical-enrichment scenario and the relative ages of different stellar populations. The Astrophysical Journal, 746(1): 14, pp. 1-12. doi:10.1088/0004-637X/746/1/14.

Cite as: https://hdl.handle.net/11858/00-001M-0000-000F-A647-5

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