Resistive MHD Simulations of Star-Disk-Jet System

Details Resistive MHD Simulations of Star-Disk-Jet System Resistive MHD Simulations of Star-Disk-Jet System

2009-08-18

arxiv.org/abs/0908.2538v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Proceedings paper of EAMA7 Symposium, October 2007, Fukuoka, Japan

Scientific paper

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.

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