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机译:使用超级奈奎斯特派斯蒙学,六次新的快速振荡AP星星在开普勒长Cadence数据中
Univ Sydney Sch Phys Sydney Inst Astron SIfA Sydney NSW 2006 Australia|Aarhus Univ Stellar Astrophys Ctr DK-8000 Aarhus C Denmark;
Univ Cent Lancashire Jeremiah Horrocks Inst Preston PR1 2HE Lancs England;
Univ Sydney Sch Phys Sydney Inst Astron SIfA Sydney NSW 2006 Australia|Aarhus Univ Stellar Astrophys Ctr DK-8000 Aarhus C Denmark;
Univ Sydney Sch Phys Sydney Inst Astron SIfA Sydney NSW 2006 Australia|Aarhus Univ Stellar Astrophys Ctr DK-8000 Aarhus C Denmark;
Univ Porto CAUP Inst Astrofis & Ciencias Espaco Rua Estrelas P-4150762 Porto Portugal;
Univ Cent Lancashire Jeremiah Horrocks Inst Preston PR1 2HE Lancs England;
Univ Hawaii Inst Astron 2680 Woodlawn Dr Honolulu HI 96822 USA;
NASA Exoplanet Sci Inst CALTECH IPAC Pasadena CA 91125 USA;
CALTECH Pasadena CA 91125 USA;
asteroseismology; techniques: photometric; stars: chemically peculiar; stars: oscillations;
机译:开普勒I型太阳型恒星的星震学:数据分析
机译:开普勒太阳型恒星的星震学:III。地面数据
机译:开普勒I型太阳恒星的星震学:数据分析
机译:快速振荡AP恒星的脉动和其环境的垂直结构
机译:所有Ap明星都去了哪里?附近疏散星团中Ap星的自转,化学丰度和磁场。
机译:来自中子星和星震学的引力波
机译:Kepler K2任务观测到的HD 24355:快速振荡的ap星在扭曲的四极杆模式下脉动