"The HARPS search for southern extra-solar planets. XVII Six long-period giant planets around BD -17 0063, HD 20868, HD 73267, HD 131664, HD 145377 HD 153950"
C. Moutou, M. Mayor, G. Lo Curto, S. Udry, F. Bouchy, W. Benz, C. Lovis, D. Naef, F. Pepe, D. Queloz, N.C. Santos, 2008
A&A in press (atro-ph/0810.4662)
The high residuals to the fitted orbit are mostly due to stellar activity. A long-period trend may nevertheless be present (see middle panel of the figure below) revealing the presence of an additional body in the system. More data are needed to establish its presence.
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Top: Temporal velocities and fitted orbital solution. Middle: Residuals to the fitted orbit. Bottom: Phase-folded velocities and fitted orbit. |
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(days) |
(JD - 2 400 000) |
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(km/s) |
(deg) |
(m/s) |
(M_Jup) |
(AU) |
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(m/s) |
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+/- 0.13 |
+/- 0.6 |
+/- 0.017 |
+/- 0.003 |
+/- 2.8 |
+/- 4.6 |
+/- 0.10 |
+/- 0.004 |
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Extrasolar planet page
Planet Search and Stellar Kinematics group page
Geneva observatory
University of Geneva