Energy flux determines magnetic field strength of planets and stars
- Autor
- CHRISTENSEN, Ulrich R1 ; HOLZWARTH, Volkmar1 ; REINERS, Ansgar2
[1] Max-Planck-lnstitut fur Sonnensystemforschung, Max Planck Strasse 2, 37191 Katlenburg-Lindau, Germany
[2] Institut für Astrophysik, Universität Göttingen, Friedrich Hund Platz 1, 37077 Göttingen, Germany - Fuente
Nature (London). 2009, Vol 457, Num 7226, pp 167-169, 3 p ; ref : 30 ref
- CODEN
- NATUAS
- ISSN
- 0028-0836
- Campo Científico
- Multidisciplinary
- Editor
- Nature Publishing Group, London
- País de la publicación
- United Kingdom
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Champ magnétique Convection Etoile faible masse Etoile jeune Etoile rotation Flux magnétique Loi échelle Naine brune Planète Jupiter Planète extrasolaire Rotation rapide Soleil Stratification densité Transfert énergie
- Palabra clave (in)
- Magnetic fields Convection Low-mass stars Young stars Rotating star Magnetic flux Scaling laws Brown dwarf stars Jupiter planet Extrasolar planets Rapid rotation Sun Density stratification Energy transfer
- Palabra clave (es)
- Estrella rotación Rotación rápida Estratificación densidad
- 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
- 20977335
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/nature07626 
https://dx.doi.org/10.1038/nature07626
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