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Resistive MHD Simulations of Star-Disk-Jet System

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arxiv 0908.2538 v1 pith:WPNQBC6N submitted 2009-08-18 astro-ph.SR

Miljenko Cemeljic , Hsien Shang , Tzu-Yang Chiang This is my paper · ORCID
classification astro-ph.SR
keywords resistivesimulationsstarstellarvicinityaboveaccretionclosest
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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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