Multi-order TODCOR: Application to observations taken with the CORALIE echelle spectrograph - II. A planet in the system HD 41004

被引:127
作者
Zucker, S
Mazeh, T
Santos, NC
Udry, S
Mayor, M
机构
[1] Observ Geneva, CH-1290 Sauverny, Switzerland
[2] Tel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Sch Phys & Astron, IL-69978 Tel Aviv, Israel
[3] Univ Lisbon, Ctr Astron & Astrophys, Observ Astron Lisboa, P-1349018 Lisbon, Portugal
关键词
methods : data analysis; techniques : radial velocities; stars : binaries : spectroscopic; stars : individual : HD 41004; stars; low-mass; brown dwarfs;
D O I
10.1051/0004-6361:20040384
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In previous works we reported the detection of a brown-dwarf companion orbiting the faint stellar component of the visual binary HD 41004. This had been achieved by applying the multi-order TwO-Dimensional CORrelation (TODCOR) algorithm to CORALIE spectra. A long-term trend of the primary component had also been detected. In this paper we report follow-up observations that seem to unravel the nature of this long-term trend. The new measurements are consistent with the presence of a 2.5 M-J planet in an eccentric orbit around HD41004 A. Thus, HD41004 is a unique hierarchical system with a brown dwarf that accompanies the faint M-component, and a planet that orbits the brighter K-component.
引用
收藏
页码:695 / 698
页数:4
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