Planet-induced Stellar Pulsations in HAT-P-2's Eccentric System

Extrasolar planets on eccentric short-period orbits provide a laboratory in which to study radiative and tidal interactions between a planet and its host star under extreme forcing conditions. Studying such systems probes how the planet's atmosphere redistributes the time-varying heat flux from...

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Bibliographic Details
Main Authors:	Wit, Julien de, Lewis, Nikole K., Knutson, Heather A., Fuller, Jim, Antoci, Victoria, Fulton, Benjamin J., Laughlin, Gregory, Deming, Drake, Shporer, Avi, Batygin, Konstantin, Cowan, Nicolas B., Agol, Eric, Burrows, Adam S., Fortney, Jonathan J., Langton, Jonathan, Showman, Adam P.
Other Authors:	Univ Arizona, Lunar & Planetary Lab
Language:	en
Published:	IOP PUBLISHING LTD 2017
Subjects:	methods: numerical planet-star interactions planets and satellites: atmospheres planets and satellites: dynamical evolution and stability planets and satellites: individual (HAT-P-2b) techniques: photometric
Online Access:	http://hdl.handle.net/10150/624378 http://arizona.openrepository.com/arizona/handle/10150/624378

by Lewis, Nikole K., Knutson, Heather A., Fuller, Jim, Antoci, Victoria, Fulton, Benjamin J., Laughlin, Gregory, Deming, Drake, Shporer, Avi, Batygin, Konstantin, Cowan, Nicolas B., Agol, Eric, Burrows, Adam S., Fortney, Jonathan J., Langton, Jonathan, Showman, Adam P., de Wit, Julien
Published 2017

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Planet-induced Stellar Pulsations in HAT-P-2's Eccentric System

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