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The formation of collimated outflows and concentric rings in magnetized Planetary Nebulae

Magnetic elds and wind asymmetries from rotating stars, along with precession of the stellar rotation axis, cancreate most of the observed Planetary Nebulae morphologies and collimated outows (jets). The collimation ofthe ows by magnetic tension becomes very ecient after the magnetized wind has pass...

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Bibliografske podrobnosti
izdano v:Revista Mexicana de Astronomía y Astrofísica
Main Authors: G. García Segura, J. A. López, J. Franco, S. Kurtz
Format: Artigo
Jezik:Inglês
Izdano: Universidad Nacional Autónoma de México 2002
Teme:
Online dostop:https://www.redalyc.org/articulo.oa?id=57112041
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