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Energy flux determines magnetic field strength

The article reports a scaling law for rapidly rotating stars that have strong density statification and predicts that the field strength of rapidly rotating brown dwarfs and massive extrasolar planets are high enough to make them observable.

Dettagli Bibliografici
Autore principale: Christensen, Ulrich R. Et. Al
Lingua:Undetermined
Soggetti:

University of Kerala

Dettagli sul posseduto da University of Kerala