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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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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2002
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57112041 |
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