The formation of collimated outflows and concentric rings in magnetized Planetary Nebulae
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| Formato: | Artículo científico |
| Lenguaje: | en |
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Universidad Nacional Autónoma de México
2002
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| _version_ | 1876463814028820480 |
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| author | G. García Segura |
| author_facet | G. García Segura |
| contents | The formation of collimated outflows and concentric rings in magnetized Planetary Nebulae G. García Segura J. A. López J. Franco S. Kurtz Física, Astronomía y Matemáticas PLANE STARS: AGB ISM: BUBBLES HYDRODYNAMICS TARY NEBULAE: GENERAL 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 passed through the reverseshock of the PN. Also, the concentric rings observed in some PNe can be explained by a solar-like magneticcycle with periodic polarity inversions. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112041 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12 |
| format | Artículo científico |
| id | redalyc_57112041 |
| institution | Redalyc |
| language | en |
| publishDate | 2002 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | The formation of collimated outflows and concentric rings in magnetized Planetary Nebulae G. García Segura Física, Astronomía y Matemáticas PLANE STARS: AGB ISM: BUBBLES HYDRODYNAMICS TARY NEBULAE: GENERAL The formation of collimated outflows and concentric rings in magnetized Planetary Nebulae G. García Segura J. A. López J. Franco S. Kurtz Física, Astronomía y Matemáticas PLANE STARS: AGB ISM: BUBBLES HYDRODYNAMICS TARY NEBULAE: GENERAL 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 passed through the reverseshock of the PN. Also, the concentric rings observed in some PNe can be explained by a solar-like magneticcycle with periodic polarity inversions. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112041 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12 |
| title | The formation of collimated outflows and concentric rings in magnetized Planetary Nebulae |
| topic | Física, Astronomía y Matemáticas PLANE STARS: AGB ISM: BUBBLES HYDRODYNAMICS TARY NEBULAE: GENERAL |
| url | https://www.redalyc.org/articulo.oa?id=57112041 |