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机译:开普勒太阳型恒星的星震学:II。恒星造型
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder Colorado 80307, USA;
Centro de Astrofísica and DFA-Faculdade de Ciências, Universidade do Porto, Portugal;
School of Mathematics and Statistics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, UK;
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK;
Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA;
INAF Osservatorio Astrofisico di Catania, Via S.Sofia 78, 95123, Catania, Italy;
INAF-IASF, Istituto di Astrofisica Spaziale e Fisica Cosmica, via del Fosso del Cavaliere 100, 00133 Roma, Italy;
Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark;
Geneva Observatory, University of Geneva, Maillettes 51, 1290, Sauverny, Switzerland;
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK|Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark;
Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006, Australia;
stars: individual (KIC 11026764); stars: interiors; stars: late-type; stars: oscillations;
机译:开普勒太阳型恒星的星震学:II。恒星造型
机译:用开普勒II观测到的太阳型恒星上的超耀斑。超耀光恒星的光度变异性:恒星旋转和星点的标志
机译:与NASA开普勒任务合奏太阳型恒星的星体地震学
机译:开普勒ZZ CETI恒星与完全进化模型的集体学
机译:恒星族调查:太阳型恒星的多样性。
机译:切趾开普勒周期图用于分离行星和恒星活动信号
机译:具有开普勒II的太阳型恒星的星震学:恒星建模