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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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http://pubman.mpdl.mpg.de/cone/persons/resource/persons26329

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