A Stringent Test of Magnetic Models of Stellar Evolution

A Stringent Test of Magnetic Models of Stellar Evolution

Main-sequence stars with convective envelopes often appear larger and cooler than predicted by standard models of stellar evolution for their measured masses. This is believed to be caused by stellar activity. In a recent study, accurate measurements were published for the K-type components of the 1...

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Bibliographic Details
Main Authors: Guillermo Torres, Gregory A. Feiden, Andrew Vanderburg, Jason L. Curtis
Format: Article
Language:English
Published: MDPI AG 2021-12-01
Series:Galaxies
Subjects:
stellar evolution
eclipsing binaries
fundamental stellar parameters
stellar activity
magnetic fields
open clusters
Online Access:https://www.mdpi.com/2075-4434/10/1/3

Internet

https://www.mdpi.com/2075-4434/10/1/3

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