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arXiv · 0908.2538

Resistive MHD Simulations of Star-Disk-Jet System

Miljenko Cemeljic·Hsien Shang·Tzu-Yang Chiang
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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.

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Miljenko Cemeljic, Hsien Shang, Tzu-Yang Chiang. 2009-08-18. Resistive MHD Simulations of Star-Disk-Jet System. https://arxiv.org/abs/0908.2538

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