Please use this identifier to cite or link to this item: http://hdl.handle.net/10773/16175
Title: The SOPHIE search for northern extrasolar planets: X. Detection and characterization of giant planets by the dozen
Author: Hébrard, G.
Arnold, L.
Forveille, T.
Correia, A. C. M.
Laskar, J.
Bonfils, X.
Boisse, I.
Díaz, R. F.
Hagelberg, J.
Sahlmann, J.
Santos, N. C.
Astudillo-Defru, N.
Borgniet, S.
Bouchy, F.
Bourrier, V.
Courcol, B.
Delfosse, X.
Deleuil, M.
Demangeon, O.
Ehrenreich, D.
Gregorio, J.
Jovanovic, N.
Labrevoir, O.
Lagrange, A.-M.
Lovis, C.
Lozi, J.
Moutou, C.
Montagnier, G.
Pepe, F.
Rey, J.
Santerne, A.
Ségransan, D.
Udry, S.
Vanhuysse, M.
Vigan, A.
Wilson, P. A.
Keywords: Planetary systems
Techniques: radial velocities
Techniques: photometric
Issue Date: Apr-2016
Publisher: EDP Sciences
Abstract: We present new radial velocity measurements of eight stars that were secured with the spectrograph SOPHIE at the 193 cm telescope of the Haute-Provence Observatory. The measurements allow detecting and characterizing new giant extrasolar planets. The host stars are dwarfs of spectral types between F5 and K0 and magnitudes of between 6.7 and 9.6; the planets have minimum masses Mp sin i of between 0.4 to 3.8 MJup and orbitalperiods of several days to several months. The data allow only single planets to be discovered around the first six stars (HD 143105, HIP 109600, HD 35759, HIP 109384, HD 220842, and HD 12484), but one of them shows the signature of an additional substellar companion in the system. The seventh star, HIP 65407, allows the discovery of two giant planets that orbit just outside the 12:5 resonance in weak mutual interaction. The last star, HD 141399, was already known to host a four-planet system; our additional data and analyses allow new constraints to be set on it. We present Keplerian orbits of all systems, together with dynamical analyses of the two multi-planet systems. HD 143105 is one of the brightest stars known to host a hot Jupiter, which could allow numerous follow-up studies to be conducted even though this is not a transiting system. The giant planets HIP 109600b, HIP 109384b, and HD 141399c are located in the habitable zone of their host star.
Peer review: yes
URI: http://hdl.handle.net/10773/16175
DOI: 10.1051/0004-6361/201527585
ISSN: 0004-6361
Appears in Collections:CIDMA - Artigos
DFis - Artigos
GGDG - Artigos

Files in This Item:
File Description SizeFormat 
HD141399.pdfmain article7.42 MBAdobe PDFView/Open


FacebookTwitterDeliciousLinkedInDiggGoogle BookmarksMySpace
Formato BibTex MendeleyEndnote Degois 

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.