KELT-9 b’s Asymmetric TESS Transit Caused by Rapid Stellar Rotation and Spin–Orbit Misalignment

KELT-9 b’s Asymmetric TESS Transit Caused by Rapid Stellar Rotation and Spin–Orbit Misalignment

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© 2020. The American Astronomical Society. All rights reserved KELT-9 b is an ultra-hot Jupiter transiting a rapidly rotating, oblate early-A-type star in a polar orbit. We model the effect of rapid stellar rotation on KELT-9 b's transit light curve using photometry from the Transiting Exoplane...

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Bibliographic Details
Main Authors: Ahlers, John P, Johnson, Marshall C, Stassun, Keivan G, Colón, Knicole D, Barnes, Jason W, Stevens, Daniel J, Beatty, Thomas, Gaudi, B Scott, Collins, Karen A, Rodriguez, Joseph E, Ricker, George, Vanderspek, Roland, Latham, David, Seager, Sara, Winn, Joshua, Jenkins, Jon M, Caldwell, Douglas A, Goeke, Robert F, Osborn, Hugh P, Paegert, Martin, Rowden, Pam, Tenenbaum, Peter
Format: Article
Language:English
Published: American Astronomical Society 2022
Online Access:https://hdl.handle.net/1721.1/134072.2
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https://hdl.handle.net/1721.1/134072.2

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