J/A+A/519/A10ivo://CDS.VizieR/J/A+A/519/A10doi:10.26093/cds/vizier.35190010CDSCouetdic J.Laskar J.Correia A.C.M.Mayor M.Udry S.2017-06-19T07:57:06Z2010-09-08T14:08:36ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmultiple-starssolar-system-planetsradial-velocityLong-term, precise Doppler measurements with the CORALIE spectrograph have revealed the presence of two massive companions to the solar-type star HD 202206. Although the three-body fit of the system is unstable, it was shown that a 5:1 mean motion resonance exists close to the best fit, where the system is stable. It was also hinted that stable solutions with a wide range of mutual inclinations and low O-C were possible. We present here an extensive dynamical study of the HD 202206 system, aiming at constraining the inclinations of the two known companions, from which we derive possible value ranges for the companion masses.2010A&A...519A..10Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/519/A10CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/390/267 : The CORALIE survey for extrasolar planets. VIII (Udry+, 2002)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/519/A10https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/519/A10http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/519/A10https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/519/A10https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/519/A10http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/519/A10GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/519/A10/hd202206Radial velocity taken with CORALIE spectrographrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJulian Date of Observationdtime.epochdoubleRVRadial Velocity of the starkm/sspect.dopplerVeloc;pos.heliocentricdoublee_RVRadial Velocity errorkm/sstat.errordouble