Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission

被引:259
|
作者
Chaplin, W. J. [1 ]
Kjeldsen, H. [2 ]
Christensen-Dalsgaard, J. [2 ]
Basu, S. [3 ]
Miglio, A. [1 ,4 ]
Appourchaux, T. [5 ]
Bedding, T. R. [6 ]
Elsworth, Y. [1 ]
Garcia, R. A. [7 ]
Gilliland, R. L. [8 ]
Girardi, L. [9 ]
Houdek, G. [10 ]
Karoff, C. [2 ]
Kawaler, S. D. [11 ]
Metcalfe, T. S. [12 ]
Molenda-Zakowicz, J. [13 ]
Monteiro, M. J. P. F. G. [14 ,15 ]
Thompson, M. J. [12 ]
Verner, G. A. [1 ,16 ]
Ballot, J. [17 ]
Bonanno, A. [18 ]
Brandao, I. M. [14 ,15 ]
Broomhall, A-M [1 ]
Bruntt, H. [2 ]
Campante, T. L. [2 ,14 ,15 ]
Corsaro, E. [18 ]
Creevey, O. L. [19 ,20 ]
Dogan, G. [2 ]
Esch, L. [3 ]
Gai, N. [3 ,21 ]
Gaulme, P. [5 ]
Hale, S. J. [1 ]
Handberg, R. [2 ]
Hekker, S. [1 ,22 ]
Huber, D. [6 ]
Jimenez, A. [19 ,20 ]
Mathur, S. [12 ]
Mazumdar, A. [23 ]
Mosser, B. [24 ]
New, R. [25 ]
Pinsonneault, M. H. [26 ]
Pricopi, D. [27 ]
Quirion, P-O [28 ]
Regulo, C. [19 ,20 ]
Salabert, D. [19 ,20 ]
Serenelli, A. M. [29 ]
Aguirre, V. Silva [30 ]
Sousa, S. G. [14 ,15 ]
Stello, D. [6 ]
Stevens, I. R. [1 ]
机构
[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[2] Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark
[3] Yale Univ, Dept Astron, New Haven, CT 06520 USA
[4] Univ Liege, Dept Astrophys Geophys & Oceanog, B-4000 Liege 1, Belgium
[5] Univ Paris 11, CNRS, UMR8617, Inst Astrophys Spatiale, F-91405 Orsay, France
[6] Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia
[7] Univ Paris Diderot, Inst Rech Lois Fondamentales Univers, Lab Astrophys Instrumentat & Modelisat, Direct Sci Mat,CEA,CNRS,Serv Astrophys,Ctr Saclay, F-91191 Gif Sur Yvette, France
[8] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[9] Ist Nazl Astrofis INAF, Osservatorio Astron Padova, I-35122 Padua, Italy
[10] Univ Vienna, Inst Astron, A-1180 Vienna, Austria
[11] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA
[12] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[13] Univ Wroclaw, Astron Inst, PL-51622 Wroclaw, Poland
[14] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal
[15] Univ Porto, Fac Ciencias, P-4150762 Oporto, Portugal
[16] Univ London, Astron Unit, London E1 4NS, England
[17] Univ Toulouse, CNRS, Inst Rech Astrophys & Planetol, F-31400 Toulouse, France
[18] INAF Osservatorio Astrofis Catania, I-95123 Catania, Italy
[19] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
[20] Inst Astrofis Canarias, E-38200 Tenerife, Spain
[21] Dezhou Univ, Dept Phys, Dezhou 253023, Peoples R China
[22] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1090 GE Amsterdam, Netherlands
[23] Homi Bhabha Ctr Sci Educ, Bombay 400088, Maharashtra, India
[24] Univ Paris 07, Univ Paris 06, Lab Etud Spatiales & Instrumentat Astrophys, Observ Paris,CNRS, F-92195 Meudon, France
[25] Sheffield Hallam Univ, Fac Arts Comp Engn & Sci, Mat Engn Res Inst, Sheffield S1 1WB, S Yorkshire, England
[26] Ohio State Univ, Dept Astron, McPherson Lab 4055, Columbus, OH 43210 USA
[27] Acad Romana, Astron Inst, RO-40557 Bucharest, Romania
[28] Canadian Space Agcy, St Hubert, PQ J3Y 8Y9, Canada
[29] Fac Ciencies, Inst Estudis Espacials Catalunya, Inst Ciencias Espacio, Bellaterra 08193, Spain
[30] Max Planck Inst Astrophys, D-85741 Garching, Germany
[31] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[32] Las Cumbres Observ Global Telescope, Goleta, CA 93117 USA
[33] NASA, Ames Res Ctr, SETI Inst, Moffett Field, CA 94035 USA
[34] NASA, Ames Res Ctr, Bay Area Environm Res Inst, Moffett Field, CA 94035 USA
[35] NASA, Ames Res Ctr, Orbital Sci Corp, Moffett Field, CA 94035 USA
关键词
SUN-LIKE STAR; RED GIANTS; OSCILLATIONS; COROT; AMPLITUDES; ISOCHRONES; RADIUS; CYCLE; DEEP;
D O I
10.1126/science.1201827
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
In addition to its search for extrasolar planets, the NASA Kepler mission provides exquisite data on stellar oscillations. We report the detections of oscillations in 500 solar-type stars in the Kepler field of view, an ensemble that is large enough to allow statistical studies of intrinsic stellar properties (such as mass, radius, and age) and to test theories of stellar evolution. We find that the distribution of observed masses of these stars shows intriguing differences to predictions from models of synthetic stellar populations in the Galaxy.
引用
收藏
页码:213 / 216
页数:4
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