Constraining Stellar Rotation at the Zero-age Main Sequence with TESS

Constraining Stellar Rotation at the Zero-age Main Sequence with TESS

The zero-age main sequence (ZAMS) is a critical phase for stellar angular momentum evolution, as stars transition from contraction-dominated spin-up to magnetic wind-dominated spin-down. We present the first robust observational constraints on rotation for FGK stars at ≈40 Myr. We have analyzed TESS...

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Bibliographic Details
Main Authors: S. T. Douglas, P. A. Cargile, S. P. Matt, A. A. Breimann, J. A. Pérez Chávez, C. X. Huang, N. J. Wright, G. Zhou
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Stellar rotation
Stellar evolution
Late-type stars
Open star clusters
Online Access:https://doi.org/10.3847/1538-4357/ad0fe3

Internet

https://doi.org/10.3847/1538-4357/ad0fe3

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