Structured, Dynamo Driven Stellar and Disc Winds

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dc.creatorvon Rekowski, Brigitta
dc.creatorBrandenburg, Axel
dc.date2003-10-15
dc.date.accessioned2026-07-07T02:10:26Z
dc.date.available2026-07-07T02:10:26Z
dc.descriptionConsiderable progress has been made in understanding the hydrodynamics, but only to a certain extent the magnetohydrodynamics, of shaping bipolar outflows forming protoplanetary nebulae (PPNs) and planetary nebulae (PNs). In particular, Blackman et al. (2001b,2001a) point out two problems related to the formation of PNs and PPNs, regarding the formation of multipolar structures and the origin of the nebulae. They propose a solution by giving a semi-quantitative physical model which should be investigated by numerical simulations.
dc.description4 pages, 6 figures, APN3 conference proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0310398
dc.identifierhttp://arxiv.org/abs/astro-ph/0310398
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6739
dc.subjectAstrophysics
dc.titleStructured, Dynamo Driven Stellar and Disc Winds
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