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Constraints on Magnetic Braking from the G8 Dwarf Stars 61 UMa and τ Cet

During the first half of their main-sequence lifetimes, stars rapidly lose angular momentum to their magnetized winds, a process known as magnetic braking. Recent observations suggest a substantial decrease in the magnetic braking efficiency when stars reach a critical value of the Rossby number, th...

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Principais autores: Travis S. Metcalfe, Klaus G. Strassmeier, Ilya V. Ilyin, Jennifer L. van Saders, Thomas R. Ayres, Adam J. Finley, Oleg Kochukhov, Pascal Petit, Victor See, Keivan G. Stassun, Sandra V. Jeffers, Stephen C. Marsden, Julien Morin, Aline A. Vidotto
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Assuntos:
Spectropolarimetry
Stellar evolution
Stellar magnetic fields
Stellar rotation
Stellar winds
Acceso en liña:https://doi.org/10.3847/2041-8213/acce38
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