4.6 Article

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

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ASTRONOMY & ASTROPHYSICS
卷 426, 期 2, 页码 695-698

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E D P SCIENCES
DOI: 10.1051/0004-6361:20040384

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methods : data analysis; techniques : radial velocities; stars : binaries : spectroscopic; stars : individual : HD 41004; stars : low-mass, brown dwarfs

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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.

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