Launching of resistive magnetic protostellar jets

Details Launching of resistive magnetic protostellar jets Launching of resistive magnetic protostellar jets

2003-11-03

arxiv.org/abs/astro-ph/0311057v1

Astronomy and Astrophysics

Astrophysics

To appear in: Stars as Suns: Activity, Evolution and Planets, eds. A. K. Dupree, A. Benz, IAU Symposium no. 219 Proceedings

Scientific paper

Turbulent accretion disks are the most probable origin of jets from young stellar objects. Using an extended version of ZEUS-3D code in the axisymmetry option we investigate the evolution of a disk wind into a collimated jet. Resistive jets propagate slower with increasing magnetic diffusivity, and the degree of collimation decreases. The resistive disk included in the simulations ejects persistent, well collimated jet.

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