Examining the Rotation Period Distribution of the 40 Myr Tucana–Horologium Association with TESS

Examining the Rotation Period Distribution of the 40 Myr Tucana–Horologium Association with TESS

The Tucana–Horologium association (Tuc-Hor) is a 40 Myr old moving group in the southern sky. In this work, we measure the rotation periods of 313 Tuc-Hor objects with TESS light curves derived from TESS full-frame images and membership lists driven by Gaia EDR3 kinematics and known youth indicators...

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Podrobná bibliografie
Hlavní autoři: Mark Popinchalk, Jacqueline K. Faherty, Jason L. Curtis, Jonathan Gagné, Daniella C. Bardalez Gagliuffi, Johanna M. Vos, Andrew Ayala, Lisseth Gonzales, Rocio Kiman
Médium: Článek
Jazyk:English
Vydáno: IOP Publishing 2023-01-01
Edice:The Astrophysical Journal
Témata:
Stellar rotation
M dwarf stars
Light curves
Young stellar objects
Young star clusters
On-line přístup:https://doi.org/10.3847/1538-4357/acb055

Internet

https://doi.org/10.3847/1538-4357/acb055

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