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The subgiant branch of ω Centauri seen through high-resolution spectroscopy - II. The most metal-rich population

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Sbordone,  L.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Pancino, E., Mucciarelli, A., Bonifacio, P., Monaco, L., & Sbordone, L. (2011). The subgiant branch of ω Centauri seen through high-resolution spectroscopy - II. The most metal-rich population. Astronomy & Astrophysics, 534: A53, pp. 1-10. doi:10.1051/0004-6361/201117378.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-3A61-E
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