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...

书目详细资料
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
格式:	文件
语言:	English
出版:	American Astronomical Society 2021
在线阅读:	https://hdl.handle.net/1721.1/134072

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