Dynamos in asymptotic-glant-branch stars as the origin of magnetic fields shaping planetary nebulae
- Autor
- BLACKMAN, Eric G1 ; FRANK, Adam1 ; MARKIEL, J. Andrew2 ; THOMAS, John H1 3 ; VAN HORN, Hugh M1
[1] Department of Physics and Astronomy and C. E. K. Mees Observatory, University of Rochester, Rochester, New York 14627-0171, United States
[2] Department of Astronomy, University of Washington, Seattle, Washington 98195-1580, United States
[3] Department of Mechanical Engineering, University of Rochester, Rochester, New York 14627-0171, United States - Fuente
Nature (London). 2001, Vol 409, Num 6819, pp 485-487 ; ref : 32 ref
- CODEN
- NATUAS
- ISSN
- 0028-0836
- Campo Científico
- Multidisciplinary
- Editor
- Nature Publishing, London
- País de la publicación
- United Kingdom
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Branche géante asymptotique Champ magnétique Ecoulement bipolaire Nébuleuse planétaire Structure interne stellaire Théorie dynamo Vent stellaire
- Palabra clave (in)
- Asymptotic giant branch Magnetic fields Bipolar flow Planetary nebulae Stellar interiors Dynamo theory Stellar winds
- Palabra clave (es)
- Rama gigante asintótica Flujo bipolar
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10L Magnetic and electric fields. Polarization of starlight
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 871849
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1038/35054008 
https://dx.doi.org/10.1038/35054008
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