The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201

Measuring the obliquities of stars hosting giant planets may shed light on the dynamical history of planetary systems. Significant efforts have been made to measure the obliquities of FGK stars with hot Jupiters, mainly based on observations of the Rossiter–McLaughlin effect. In contrast, M dwarfs w...

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發表在:	The Astrophysical Journal Letters
Main Authors:	Tianjun Gan, Sharon X. Wang, Fei Dai, Joshua N. Winn, Shude Mao, Siyi Xu, Enric Pallé, Jacob L. Bean, Madison Brady, Nina Brown, Cicero Lu, Rafael Luque, Teo Mocnik, Andreas Seifahrt, Guđmundur K. Stefánsson
格式:	Article
語言:	英语
出版:	IOP Publishing 2024-01-01
主題:	Planetary alignment Exoplanet dynamics Star-planet interactions Exoplanets M dwarf stars Hot Jupiters
在線閱讀:	https://doi.org/10.3847/2041-8213/ad5967