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Multiple stellar populations in the massive clusters M22 and Omega Centauri
Published online by Cambridge University Press: 05 March 2015
Abstract
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.
- 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