机译:重力主导的混合模式揭示了红巨星的快速核旋转
InstituutvoorSterrenkunde, KatholiekeUniversiteitLeuven,3001 Leuven, Belgium;
Institutd'Astrophysiqueetde Geophysiquedel'UniversitedeLiege,4000 Liege,Belgium;
InstituutvoorSterrenkunde, KatholiekeUniversiteitLeuven,3001 Leuven, Belgium,InstitutfiirAstronomieder Universitat Wien, Tiirkenschanzstra Be 17,1180 Wien, Austria,InstituutvoorSterrenkunde, KatholiekeUniversiteitLeuven,3001 Leuven, Belgium;
InstituutvoorSterrenkunde, KatholiekeUniversiteitLeuven,3001 Leuven, Belgium,Afdeling Sterrenkunde, Institute for Mathematics Astrophysics and Particle Physics (IMAPP), Radboud University Nijmegen, 6500GL Nijmegen, The Netherlands;
Laboratoire Astrophysique, Instrumentation et Moderation (AIM), CEA/DSM-CNRS-Universite Paris Diderot;
Institutde Recherche sur les lois Fondamentalesde I'Univers/ Service d'Astrophysique (IRFU/Sap), Centre de Saclay, 91191 Gif-sur-Yvette Cedex, France;
Astronomical Institute 'Anton Pannekoek, University of Amsterdam, Science Park 904,1098 XH Amsterdam,The Netherlands,School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B152TT, UK;
Institutd'Astrophysiqueetde Geophysiquedel'UniversitedeLiege,4000 Liege,Belgium;
Laboratoire d'etudes spatiales etd'instrumentation (LESIA), CNRS, Universite Pierre et Marie Curie, Universite Denis Diderot, Observatoi rede Paris, 92195 Meudon Cedex, France;
Observatoirede Geneve, Universite de Geneve, 51 Ch.des Maillettes, 1290 Sauverny, Switzerland;
Sydney Institute for Astronomy (SlfA), School of Physics, University of Sydney 2006, Australia;
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B152TT, UK;
Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark;
InstituutvoorSterrenkunde, KatholiekeUniversiteitLeuven,3001 Leuven, Belgium;
InstituutvoorSterrenkunde, KatholiekeUniversiteitLeuven,3001 Leuven, Belgium;
Department of Astronomy and Physics, Saint Marys University, Halifax, NS B3H 3C3, Canada;
Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark;
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B152TT, UK;
Institutd'Astrophysiqueetde Geophysiquedel'UniversitedeLiege,4000 Liege,Belgium;
Sydney Institute for Astronomy (SlfA), School of Physics, University of Sydney 2006, Australia;
Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark;
Orbital Sciences Corporation/NASA Ames Research Center, Moffett Field, 94035 California, USA;
Orbital Sciences Corporation/NASA Ames Research Center, Moffett Field, 94035 California, USA;
Orbital Sciences Corporation/NASA Ames Research Center, Moffett Field, 94035 California, USA;
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机译:重力主导的混合模式揭示了红巨星的快速核旋转