Launching of resistive magnetic protostellar jets

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dc.creatorCemeljic, Miljenko
dc.creatorFendt, Christian
dc.date2003-11-03
dc.date.accessioned2026-07-07T02:11:02Z
dc.date.available2026-07-07T02:11:02Z
dc.descriptionTurbulent 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.
dc.descriptionTo appear in: Stars as Suns: Activity, Evolution and Planets, eds. A. K. Dupree, A. Benz, IAU Symposium no. 219 Proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0311057
dc.identifierhttp://arxiv.org/abs/astro-ph/0311057
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6940
dc.subjectAstrophysics
dc.titleLaunching of resistive magnetic protostellar jets
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