J/A+A/542/A78ivo://CDS.VizieR/J/A+A/542/A78doi:10.26093/cds/vizier.35420078CDSZasche P.Uhlar R.Slechta M.Wolf M.Harmanec P.Nemravova J.A.,Korcakova D.2017-06-19T07:58:15Z2012-06-12T10:49:23ZCDS support team

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

cds-question@unistra.frmultiple-starseclipsing-binary-starsradial-velocityinfrared-photometryvisible-astronomybroad-band-photometryThe study of stellar multiple systems provides us with important information about the stellar formation processes and can help us to estimate the multiplicity fraction in the Galaxy. 65 UMa belongs to a rather small group of stellar systems of higher multiplicity, whose inner and outer orbits are well-known. This allows us to study the long-term stability and evolution of the orbits in these systems. We obtained new photometric and spectroscopic data that when combined with interferometric data enables us to analyze the system 65 UMa and determine its basic physical properties.2012A&A...542A..78Zhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/542/A78CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/542/A78https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/542/A78http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/542/A78https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/542/A78https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/542/A78http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/542/A78GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/A+A/542/A78/astromThe astrometry of 65 UMa used for the analysisrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDateDate of observationyrtime.epochdoublerhoAngular separation of the componentsarcsecpos.angDistancefloatphiPosition angle between the componentsdegpos.posAngfloatRefReference/Observermeta.ref;pos.framecharJ/A+A/542/A78/minimaHeliocentric minima times of 65 UMa used for the analysise_HJD? Error of HJDdstat.error;time.epochdoublenullableP/S[Prim Sec] Type of Minimum (primary/secondary)meta.codecharFilterFilter(s) Usedinstr.bandpasscharRefReference/Observermeta.ref;pos.framecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHJDHeliocentric Julian Date of Minimumdtime.epochdoubleJ/A+A/542/A78/photBVRI photometry of 65 UMaHJDHeliocentric Julian Date of Observationdtime.epochdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBand[BVRI] Observed bandinstr.bandpasscharmagMagnitude in Band Filtermagphot.magfloate_magError of magnitudemagstat.error;phot.magfloatJ/A+A/542/A78/rvRadial velocities of 65 UMarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHJDHeliocentric Julian Date of Observationdtime.epochdoubleRV1oOriginal velocity of the primary componentkm/sphys.veloc;pos.heliocentricfloatRV2oOriginal velocity of the secondary componentkm/sphys.veloc;pos.heliocentricfloatRV3Velocity of the third componentkm/sphys.veloc;pos.heliocentricfloatRV1cCorrected velocity of the primary component (640-day orbit subtracted)km/sphys.veloc;pos.heliocentricfloatRV2cCorrected velocity of the secondary component (640-day orbit subtracted)km/sphys.veloc;pos.heliocentricfloat