The Orbit of Warm Jupiter WASP-106 b is Aligned with its Star

The Orbit of Warm Jupiter WASP-106 b is Aligned with its Star

Understanding orbital obliquities, or the misalignment angles between a star’s rotation axis and the orbital axis of its planets, is crucial for unraveling the mechanisms of planetary formation and migration. In this study, we present an analysis of Rossiter–McLaughlin (RM) observations of the warm...

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Bibliographic Details
Main Authors: Jan-Vincent Harre, Alexis M. S. Smith, Teruyuki Hirano, Szilárd Csizmadia, Amaury H. M. J. Triaud, David R. Anderson
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astronomical Journal
Subjects:
Exoplanet evolution
Exoplanet migration
Radial velocity
Photometry
Transits
Online Access:https://doi.org/10.3847/1538-3881/acf46d

Internet

https://doi.org/10.3847/1538-3881/acf46d

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