SPIN-ORBIT ALIGNMENT OF EXOPLANET SYSTEMS: ENSEMBLE ANALYSIS USING ASTEROSEISMOLOGY

The angle ψ between a planet's orbital axis and the spin axis of its parent star is an important diagnostic of planet formation, migration, and tidal evolution. We seek empirical constraints on ψ by measuring the stellar inclination i[subscript s] via asteroseismology for an ensemble of 25 sola...

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Main Authors: Campante, T. L. (Author), Lund, M. N. (Author), Kuszlewicz, J. S. (Author), Davies, G. R. (Author), Chaplin, W. J. (Author), Albrecht, S. (Author), Bedding, T. R. (Author), Benomar, O. (Author), Bossini, D. (Author), Handberg, R. (Author), Santos, A. R. G. (Author), Basu, S. (Author), Christensen-Dalsgaard, J. (Author), Elsworth, Y. P. (Author), Hekker, S. (Author), Hirano, T. (Author), Huber, D. (Author), Karoff, C. (Author), Kjeldsen, H. (Author), Lundkvist, M. S. (Author), North, T. S. H. (Author), Silva Aguirre, V. (Author), Stello, D. (Author), White, T. R. (Author), Winn, Joshua Nathan (Contributor), Van Eylen, Vincent (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2016-05-24T00:46:33Z.
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