Asteroseismology of the Hyades with K2: first detection of main-sequence solar-like oscillations in an open cluster

被引:18
|
作者
Lund, Mikkel N. [1 ,2 ]
Basu, Sarbani [3 ]
Aguirre, Victor Silva [2 ]
Chaplin, William J. [1 ,2 ]
Serenelli, Aldo M. [4 ]
Garcia, Rafael A. [5 ]
Latham, David W. [6 ]
Casagrande, Luca [7 ]
Bieryla, Allyson [6 ]
Davies, Guy R. [1 ,2 ]
Viani, Lucas S. [3 ]
Buchhave, Lars A. [8 ,9 ]
Miglio, Andrea [1 ,2 ]
Soderblom, David R. [10 ]
Valenti, Jeff A. [10 ]
Stefanik, Robert P. [6 ]
Handberg, Rasmus [2 ]
机构
[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[2] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
[3] Yale Univ, Dept Astron, POB 208101, New Haven, CT 06520 USA
[4] Inst Space Sci CSIC IEEC, Campus UAB,Carrer Can Magrans S-N, E-08193 Cerdanyola Del Valles, Barcelona, Spain
[5] Univ Paris Diderot, CNRS, CEA DRF, Lab AIM,IRFU SAp,Ctr Saclay, F-91191 Gif Sur Yvette, France
[6] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[7] Australian Natl Univ, Mt Stromlo Observ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[8] Univ Copenhagen, Nat Hist Museum Denmark, Ctr Star & Planet Format, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark
[9] Univ Copenhagen, Niels Bohr Inst, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark
[10] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
基金
新加坡国家研究基金会; 英国科学技术设施理事会; 欧洲研究理事会; 美国国家科学基金会;
关键词
asteroseismology; methods: data analysis; stars:; individual:; EPIC; 210444167; (HIP; 20357; vB; 37); 210499243; 19877; 20); stars: rotation; galaxies: star clusters: individual: Hyades; ACTIVITY-ROTATION RELATIONSHIP; HERTZSPRUNG-RUSSELL DIAGRAMS; STELLAR EVOLUTION DATABASE; GENEVA-COPENHAGEN SURVEY; SUN-LIKE STAR; M-CIRCLE-DOT; MAGNETIC ACTIVITY; RED GIANTS; NGC; 6791; F-STARS;
D O I
10.1093/mnras/stw2160
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Hyades open cluster was targeted during Campaign 4 (C4) of the NASA K2 mission, and short-cadence data were collected on a number of cool main-sequence stars. Here, we report results on two F-type stars that show detectable oscillations of a quality that allows asteroseismic analyses to be performed. These are the first ever detections of solar-like oscillations in main-sequence stars in an open cluster.
引用
收藏
页码:2600 / 2611
页数:12
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