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Multiple stellar populations in the massive clusters M22 and Omega Centauri

Published online by Cambridge University Press:  05 March 2015

A. F. Marino
A. F. Marino*
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany email: [email protected]
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Abstract

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An intriguing discovery in the field of multiple stellar populations in globular clusters is that some of them show internal variations in the bulk of the heavy-element content. I summarize the chemical properties of one of these clusters, M22, in comparison with the most extreme ω Centauri, underlying the analogies and differences between the two objects.

Keywords

stars: abundancesglobular clusters: individual (M22, ω Centauri)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 234 - 236
Copyright
Copyright © International Astronomical Union 2015 

References

Alves-Brito, A., Yong, D., Meléndez, J., Vásquez, S., & Karakas, A. I., 2012, A&A, 540, A3Google Scholar
Da Costa, G. S., Held, E. V., Saviane, I., & Gullieuszik, M., 2009, ApJ, 705, 1481Google Scholar
Da Costa, G. S., & Marino, A. F., 2011, PASA, 28, 28Google Scholar
Marino, A. F., Milone, A. P., Piotto, G., et al., 2009, A&A, 505, 1099Google Scholar
Marino, A. F., Sneden, C., Kraft, R. P., et al., 2011a, A&A, 532, A8Google Scholar
Marino, A. F., Milone, A. P., Piotto, G., et al., 2011b, ApJ, 731, 64Google Scholar
Marino, A. F., Milone, A. P., Sneden, C., et al. 2012a, A&A, 541, A15Google Scholar
Marino, A. F., Milone, A. P., Piotto, G., et al. 2012b, ApJ, 746, 14CrossRefGoogle Scholar
Piotto, G., Milone, A. P., Anderson, J., et al., 2012, arXiv:1208.1873Google Scholar