Announced during the XIX th IAP Colloquium "Extrasolar Planets: Today & Tormorrow", Paris, June 2003
A Hierarchic quadruple system: A 2.3 M_Jup planet orbiting a K2V star + a 19 M_Jup brown dwarf orbiting a M4V star HD 41004 is a close visual binary (K2V star + M4V star; separation: 0.5 arcsec).
A 1.3-day radial-velocity signal was rapidly detected
Santos et al. 2002 (A&A 392, 215) have interpreted this signal as the result of the presence of a brown dwarf orbiting the secondary star HD 41004 B
Zucker et al. 2003 (A&A 404, 775) have detected the secondary spectrum using TODCOR (Zucker & Mazeh 1994, ApJ 420, 806), a 2-D correlation algorithm. The radial-velocity variation of the secondary spectrum has a period of 1.3 d, validating the interpretation by Santos et al.
Zucker et al. 2004 (A&A 426, 695) have finally detected a longer-period velocity variation of the primary spectrum (see the Figure below). This variation is due to the presence of a planet around the primary star
|
(days) |
(JD - 2 400 000) |
|
(km/s) |
(deg) |
(km/s) |
(M_Jup) |
(AU) |
|
(m/s) |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
Extrasolar planet page
Planet Search and Stellar Kinematics group page
Geneva observatory
University of Geneva