Rotational Evolution of Classical T Tauri Stars: Models and Observations

We developed a grid of stellar rotation models for low-mass and solar-type classical T Tauri stars (CTTS; 0.3 M _⊙ < M _* < 1.2 M _⊙ ). These models incorporate the star–disk interaction and magnetospheric ejections to investigate the evolution of the stellar rotation rate as a function of the...

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Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Javier Serna, Giovanni Pinzón, Jesús Hernández, Ezequiel Manzo-Martínez, Karina Mauco, Carlos G. Román-Zúñiga, Nuria Calvet, Cesar Briceño, Ricardo López-Valdivia, Marina Kounkel, Guy S. Stringfellow, Keivan G. Stassun, Marc Pinsonneault, Lucia Adame, Lyra Cao, Kevin Covey, Amelia Bayo, Alexandre Roman-Lopes, Christian Nitschelm, Richard R. Lane
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Subjects:
Classical T Tauri stars
Stellar evolution
Stellar magnetic fields
Stellar properties
Stellar rotation
Stellar winds
Online Access:https://doi.org/10.3847/1538-4357/ad3a6b

Internet

https://doi.org/10.3847/1538-4357/ad3a6b

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