Magnetically channeled accretion in T Tauri stars : a dynamical process
Astrophysics
2016-11-03 v1
Abstract
We review observational evidence and open issues related to the process of magnetospheric accretion in T Tauri stars. Emphasis is put on recent numerical simulations and observational results which suggest that the interaction between the stellar magnetosphere and the inner accretion disk is a highly time dependent process on timescales ranging from hours to months.
Keywords
Cite
@article{arxiv.astro-ph/0306553,
title = {Magnetically channeled accretion in T Tauri stars : a dynamical process},
author = {J. Bouvier and S. H. P. Alencar and C. Dougados},
journal= {arXiv preprint arXiv:astro-ph/0306553},
year = {2016}
}
Comments
To appear in Open Issues in Local Star Formation and Early Stellar Evolution, eds. J. Lepine, J. Gregorio-Hetem