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The nuclear path of the CNO cycles in massive stars
Published online by Cambridge University Press: 27 October 2016
Abstract
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We discuss how the nuclear path of the CNO cycles in massive stars can be employed as a quality indicator for model atmosphere analyses and for the derivation of tight observational constraints for developing a better understanding of the evolution of rotating massive stars.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 142 - 143
- Copyright
- Copyright © International Astronomical Union 2016
References
Przybilla, N., Firnstein, M., Nieva, M. F., Meynet, G., & Maeder, A.
2010, A&A, 517, A38
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