The ELODIE survey for northern extra-solar planets -: IV.: HD196885, a close binary star with a 3.7-year planet

被引:61
|
作者
Correia, A. C. M. [1 ,2 ]
Udry, S. [2 ]
Mayor, M. [2 ]
Eggenberger, A. [2 ,3 ]
Naef, D. [4 ]
Beuzit, J. -L. [3 ]
Perrier, C. [3 ]
Queloz, D. [2 ]
Sivan, J. -P. [5 ]
Pepe, F.
Santos, N. C. [2 ,6 ]
Segransan, D. [5 ]
机构
[1] Univ Aveiro, Dept Fis, P-3810193 Aveiro, Portugal
[2] Observ Geneva, CH-1290 Sauverny, Switzerland
[3] Univ Grenoble 1, Lab Astrophys Grenoble, F-38041 Grenoble, France
[4] European So Observ, Santiago 19, Chile
[5] Lab Astrophys Marseille, F-13376 Marseille, France
[6] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal
关键词
stars : individual : HD196885 A; stars : individual : HD196885 B; stars : binaries : visual; stars : planetary systems techniques : radial velocities; methods : observational;
D O I
10.1051/0004-6361:20078908
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We aim to significantly increase the number of detected extra-solar planets in a magnitude-limited sample to improve our knowledge of their orbital element distributions and thus obtain better constraints for planet-formation models. Methods. Radial-velocity data were taken at Haute-Provence Observatory (OHP, France) with the ELODIE echelle spectrograph. Results. We report the presence of a planet orbiting HD 196885 A, with an orbital period of 1349 days. This star was previously suggested to host a 386-day planet, but we cannot confirm its existence. We also detect the presence of a stellar companion, HD 196885 B, and give some constraints on its orbit.
引用
收藏
页码:271 / 275
页数:5
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