Magnetic Activity Evolution of Solar-like Stars. II. Sph–Ro Evolution of Kepler Main-sequence Targets

Magnetic Activity Evolution of Solar-like Stars. II. Sph–Ro Evolution of Kepler Main-sequence Targets

There is now a large sample of stars observed by the Kepler satellite with measured rotation periods and photometric activity index S _ph . We use this data, in conjunction with stellar interiors models, to explore the interplay of magnetism, rotation, and convection. Stellar activity proxies other...

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Bibliographic Details
Main Authors: Savita Mathur, Ângela R. G. Santos, Zachary R. Claytor, Rafael A. García, Antoine Strugarek, Adam J. Finley, Quentin Noraz, Louis Amard, Paul G. Beck, Alfio Bonanno, Sylvain N. Breton, Allan S. Brun, Lyra Cao, Enrico Corsaro, Diego Godoy-Rivera, Stéphane Mathis, Dinil B. Palakkatharappil, Marc H. Pinsonneault, Jennifer van Saders
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar analogs
Stellar types
Late-type stars
Low mass stars
Stellar oscillations
Asteroseismology
Online Access:https://doi.org/10.3847/1538-4357/adb8cc
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https://doi.org/10.3847/1538-4357/adb8cc

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