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A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars.
Stello, Dennis; Cantiello, Matteo; Fuller, Jim; Huber, Daniel; García, Rafael A; Bedding, Timothy R; Bildsten, Lars; Aguirre, Victor Silva.
Afiliação
  • Stello D; Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, Sydney, New South Wales 2006, Australia.
  • Cantiello M; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark.
  • Fuller J; Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106, USA.
  • Huber D; Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106, USA.
  • García RA; TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, California Institute of Technology, Pasadena, California 91125, USA.
  • Bedding TR; Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, Sydney, New South Wales 2006, Australia.
  • Bildsten L; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark.
  • Aguirre VS; SETI Institute, 189 Bernardo Avenue, Mountain View, California 94043, USA.
Nature ; 529(7586): 364-7, 2016 Jan 21.
Article em En | MEDLINE | ID: mdl-26727160
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Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prevalence_studies / Risk_factors_studies Idioma: En Ano de publicação: 2016 Tipo de documento: Article
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prevalence_studies / Risk_factors_studies Idioma: En Ano de publicação: 2016 Tipo de documento: Article