Pulsating stars harbouring planets

被引:1
作者
Moya, A. [1 ]
机构
[1] Ctr Astrobiol INTA CSIC, Dept Astrofis, Madrid 28691, Spain
来源
HOT PLANETS AND COOL STARS | 2013年 / 47卷
关键词
ASTEROSEISMOLOGY; PARAMETERS; TOOL;
D O I
10.1051/epjconf/20134709005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Why bother with asteroseismology while studying exoplanets? There are several answers to this question. Asteroseismology and exoplanetary sciences have much in common and the synergy between the two opens up new aspects in both fields. These fields and stellar activity, when taken together, allow maximum extraction of information from exoplanet space missions. Asteroseismology of the host star has already proved its value in a number of exoplanet systems by its unprecedented precision in determining stellar parameters. In addition, asteroseismology allows the possibility of discovering new exoplanets through time delay studies. The study of the interaction between exoplanets and their host stars opens new windows on various physical processes. In this review I will summarize past and current research in exoplanet asteroseismology and explore some guidelines for the future.
引用
收藏
页数:4
相关论文
共 38 条
  • [1] Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265
    Ballot, J.
    Gizon, L.
    Samadi, R.
    Vauclair, G.
    Benomar, O.
    Bruntt, H.
    Mosser, B.
    Stahn, T.
    Verner, G. A.
    Campante, T. L.
    Garcia, R. A.
    Mathur, S.
    Salabert, D.
    Gaulme, P.
    Regulo, C.
    Roxburgh, I. W.
    Appourchaux, T.
    Baudin, F.
    Catala, C.
    Chaplin, W. J.
    Deheuvels, S.
    Michel, E.
    Bazot, M.
    Creevey, O.
    Dolez, N.
    Elsworth, Y.
    Sato, K. H.
    Vauclair, S.
    Auvergne, M.
    Baglin, A.
    [J]. ASTRONOMY & ASTROPHYSICS, 2011, 530
  • [2] DETERMINATION OF STELLAR RADII FROM ASTEROSEISMIC DATA
    Basu, Sarbani
    Chaplin, William J.
    Elsworth, Yvonne
    [J]. ASTROPHYSICAL JOURNAL, 2010, 710 (02) : 1596 - 1609
  • [3] Seismic analysis of the planet-hosting star μ Arae
    Bazot, M
    Vauclair, S
    Bouchy, F
    Santos, NC
    [J]. ASTRONOMY & ASTROPHYSICS, 2005, 440 (02) : 615 - 621
  • [4] Boisse I., 2011, A A, V528, P4
  • [5] Bouchy F., A A, V440, P609
  • [6] Line-profile tomography of exoplanet transits - II. A gas-giant planet transiting a rapidly rotating A5 star☆
    Cameron, A. Collier
    Guenther, E.
    Smalley, B.
    McDonald, I.
    Hebb, L.
    Andersen, J.
    Augusteijn, Th.
    Barros, S. C. C.
    Brown, D. J. A.
    Cochran, W. D.
    Endl, M.
    Fossey, S. J.
    Hartmann, M.
    Maxted, P. F. L.
    Pollacco, D.
    Skillen, I.
    Telting, J.
    Waldmann, I. P.
    West, R. G.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 407 (01) : 507 - 514
  • [7] Chaplin W. J., 2010, ASTROPHYS J LETT, V713, P169
  • [8] Christensen-Dalsgaard J., 2010, ApJ, V713, P164
  • [9] Planetary detection limits taking into account stellar noise I. Observational strategies to reduce stellar oscillation and granulation effects
    Dumusque, X.
    Udry, S.
    Lovis, C.
    Santos, N. C.
    Monteiro, M. J. P. F. G.
    [J]. ASTRONOMY & ASTROPHYSICS, 2011, 525
  • [10] AN IN-DEPTH STUDY OF GRID-BASED ASTEROSEISMIC ANALYSIS
    Gai, Ning
    Basu, Sarbani
    Chaplin, William J.
    Elsworth, Yvonne
    [J]. ASTROPHYSICAL JOURNAL, 2011, 730 (02)