J/A+A/350/513ivo://CDS.VizieR/J/A+A/350/513doi:10.26093/cds/vizier.33500513CDSKahanpaa J.Jetsu L.Alha L.Ezhkova O.V.Grankin K.N.Hackman T.,Ibragimov M.A.Kokko M.Kondratiev V.B.Laakso T.Lindroos O.,Mel'nikov S.Yu.Nikula P.O.Schultz J.Shevchenko V.S.Torppa J.,Tuominen I.Tyynela J.Virtanen J.1999-10-24T21:19:14Z1999-10-24T21:18:50ZCDS support team

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

cds-question@unistra.frvariable-starsinfrared-photometryvisible-astronomybroad-band-photometryOur time series analysis of V368 Cep photometry ascertains the rotation period of 2.74d uniquely. The manifestations of starspot induced luminosity variations in this chromospherically active star include rapid light curve changes and differential rotation of about 3%. We conclude that the single rapidly rotating variable V368 Cep is a high inclination K1V post T Tauri star.1999A&A...350..513Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/350/513CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/350/513https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/350/513http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/350/513https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/350/513https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/350/513http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/350/513GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/A+A/350/513/table5The collected photometry of V368 CeprecnoRecord number assigned by the VizieR team. Should Not be used for identification.intSet[1/9] Set numberintHJDObserving timeddoubleUmag? U magnitude (1)magfloatnullableBmag? B magnitude (1)magfloatnullableVmag? V magnitude (1)magfloatnullableRmag? R magnitude (1)magfloatnullableImag? I magnitude (1)magfloatnullableFlareDetected flareschar