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Tidal evolution of stars hosting massive close-in planets
Published online by Cambridge University Press: 27 October 2016
Abstract
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Close-in massive planets transfer angular momentum to their host stars and influence their rotation through the torques associated with the tides raised on the star by the planet. For a star hosting a hot Jupiter, the limit of distance below which tidal torques cannot be neglected grows from a ~0.04 to a ~0.07 AU as the mass of the planet grows from 0.5 to 4MJup.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , pp. 57 - 62
- Copyright
- Copyright © International Astronomical Union 2016
References
Ferraz-Mello, S., Santos, M., Folonier, H., Csizmadia, S., Nascimento, J. D. D. Jr, & Pätzold, M.
2015
ApJ
807, id. 78 (arXiv: 1503.04369).CrossRefGoogle Scholar
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