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X-ray emission regimes and rotation sequences in the M34 open cluster
Published online by Cambridge University Press: 07 August 2014
Abstract
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I report on a correlation between the saturated and non-saturated regimes of X-ray emission and the rotation sequences that have been observed in the M34 open cluster. An interpretation of this correlation in term of magnetic activity evolution in the early stage of evolution on the main sequence is presented.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 106 - 109
- Copyright
- Copyright © International Astronomical Union 2014
References
Micela, G. 2002, Stellar Coronae in the Chandra and XMM-Newton Era, ASP Conference Proceedings, Vol. 277, p.263Google Scholar
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