Resistive MHD Simulations of Star-Disk-Jet System
Solar and Stellar Astrophysics
2009-08-19 v1
Abstract
Stellar magnetosphere and accretion disk interact, and a result should be outflow launched from the innermost vicinity of a protostellar object. We simulated physical conditions in this region by resistive MHD simulations. Outflows resembling the observed ones do not happen in the closest vicinity, except for quasi-stationary funnel flows onto the star, but could occur at few tens of stellar radii above the star. Numerical simulations we performed using our resistive version of ZEUS-3D code, ZEUS347.
Keywords
Cite
@article{arxiv.0908.2538,
title = {Resistive MHD Simulations of Star-Disk-Jet System},
author = {Miljenko Cemeljic and Hsien Shang and Tzu-Yang Chiang},
journal= {arXiv preprint arXiv:0908.2538},
year = {2009}
}
Comments
Proceedings paper of EAMA7 Symposium, October 2007, Fukuoka, Japan