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Magnetic activity in the atmospheres of F-type binaries: V963 XSCyg, XZ CMi, V965 Cyg
Published online by Cambridge University Press: 01 August 2006
Abstract
We have found photometric indications that Interacting Eclipsing Binaries of early to mid F spectral type (and possibly A) have strong magnetic activity which would arise from convective atmospheres. Light curve solutions and periodicity studies revealing spots, magnetic breaking and magnetic cycles are presented in XZ CMi, V965 Cyg and V963 Cyg.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S239: Convection in Astrophysics , August 2006 , pp. 505 - 506
- Copyright
- Copyright © International Astronomical Union 2007