Skip to Main content Skip to Navigation
Journal articles

Star/disk interaction and angular momentum evolution model for solar-like stars

Abstract : The magnetic field in young stellar object is undoubtedly the most important component when one dealing with the angular momentum evolution. It controls this latter one from the pre-main sequence, during the so-called disk locking phase where the stars magnetically interact with their surrounding disk, to the main-sequence through powerful stellar winds that remove angular momentum from the stellar surface. We present new models for the rotational evolution of solar-like stars between 1 Myr and 10 Gyr with the aim to reproduce the distributions of rotational periods observed for star forming regions and young open clusters within this age range. We based our simulation on a recent model dedicated to the study of the angular momentum evolution of solar-type stars. This model include a new wind braking law based on recent numerical simulations of magnetized stellar winds and a specific dynamo and mass-loss prescription are used to link the angular momentum loss-rate to angular velocity evolution. The model additionally allows for a core/envelope decoupling with an angular momentum transfer between these two regions. Since this former model didn't include any physical star/disk interaction description, two star/disk interaction processes are eventually added to it in order to reproduce the apparent small angular velocities to which the stellar surface is subject during the disk accretion phase. We have developed rotational evolution models for slow, median and fast rotators including two star/disk interaction scenarios that are the magnetospheric ejection and the accretion powered stellar winds processes. The models appear to fail at reproducing the rotational behaviour of solar-type stars except when a more intense magnetic field is used during the disk accretion phase.
Document type :
Journal articles
Complete list of metadata

https://hal-insu.archives-ouvertes.fr/insu-03327013
Contributor : Nathalie Pothier Connect in order to contact the contributor
Submitted on : Thursday, August 26, 2021 - 4:54:06 PM
Last modification on : Tuesday, October 19, 2021 - 7:00:49 PM
Long-term archiving on: : Saturday, November 27, 2021 - 6:41:13 PM

File

epjconf_mag2013_05007.pdf
Publisher files allowed on an open archive

Licence


Distributed under a Creative Commons Attribution 4.0 International License

Identifiers

Collections

Citation

Florian Gallet. Star/disk interaction and angular momentum evolution model for solar-like stars. EPJ Web of Conferences, EDP Sciences, 2014, 64, pp.05007. ⟨10.1051/epjconf/20136405007⟩. ⟨insu-03327013⟩

Share

Metrics

Les métriques sont temporairement indisponibles