J/A+A/542/A18ivo://CDS.VizieR/J/A+A/542/A18doi:10.26093/cds/vizier.35420018CDSLagrange A.-M.De Bondt K.Meunier N.Sterzik M.Beust H.Galland F.2017-07-04T07:09:07Z2012-08-23T07:34:41ZCDS support team

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

cds-question@unistra.frmultiple-starssolar-system-planetsradial-velocityThe {beta} Pictoris system with its debris disk and a massive giant planet orbiting at ~=9AU represents an ideal laboratory for studying giant planet formation and evolution as well as planet-disk interactions. {beta} Pic b can also help in testing brightness-mass relations at young ages. Other planets, yet undetected, may of course be present in the system. We aim at directly constraining the mass of {beta} Pic b and at searching for additional jovian planets on orbits closer than typically 2AU.2012A&A...542A..18Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/542/A18CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/299/557 : Light variations on Beta Pic (Lecavelier des Etangs+, 1995)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/542/A18https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/542/A18http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/542/A18https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/542/A18https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/542/A18http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/542/A18GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/542/A18/rvbpic{beta} Pic radial velocitiesJDJulian datedtime.epochdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRVRadial velocitykm/sphys.veloc;pos.heliocentricfloate_RVrms uncertainty on RVkm/sstat.errorfloat