J/PAZh/41/148ivo://CDS.VizieR/J/PAZh/41/148CDSArkhipova V.P.Esipov V.F.Ikonnikova N.P.Komissarova G.V.2017-06-12T08:25:15Z2015-09-08T14:19:46ZCDS support team

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

cds-question@unistra.frvariable-starsvisible-astronomyWide-band photometryspectroscopyThe photoelectric UBV observations of the peculiar symbiotic star V1329 Cyg performed at the Crimean Station of the SAI-MSU during 245 nights over the period 2003-2014 are presented. The star's light curves since 1973 from the Crimean observations are shown. The brightness decline after its outburst over the last 40 years was 0.8m-1.0m. The phase color curves at phases 0.2 and 0.8 have maxima. Their qualitative interpretation in terms of the model of interacting winds in symbiotic binary star systems is proposed. The orbital period of the binary system has been redetermined. The spectroscopic observations at the 125-cm telescope of the Crimean Station from 1994 to 2014 have confirmed the change in the system's emission spectrum with orbital phase.2015PAZh...41..148Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/41/148CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PAZh/41/148https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/41/148http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/41/148https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PAZh/41/148https://vizier.iucaa.in/viz-bin/votable?-source=J/PAZh/41/148http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PAZh/41/148GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tap2.833731416716205e-19 6.118840631666147e-19OpticaldefaultJ/PAZh/41/148/table3The equivalent widths of the emission lines in the spectrum of V1329 CygrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJulian datedtime.epochintW4340? Equivalent width of 4340 HI0.1nmspect.line.eqWidth;em.line.HIfloatnullableW4686? Equivalent width of 4686 HeII0.1nmspect.line.eqWidthfloatnullableW4861? Equivalent width of 4861 HI0.1nmspect.line.eqWidth;em.line.HIfloatnullableW5412? Equivalent width of 5412 HeII0.1nmspect.line.eqWidthfloatnullableW5876? Equivalent width of 5876 HeI0.1nmspect.line.eqWidthfloatnullableW6087? Equivalent width of 6087 [FeVII]0.1nmspect.line.eqWidthfloatnullableW6375? Equivalent width of 6375 [FeX]0.1nmspect.line.eqWidthfloatnullableW6563? Equivalent width of 6563 HI0.1nmspect.line.eqWidth;em.line.HIfloatnullableW6678? Equivalent width of 6678 HeI0.1nmspect.line.eqWidthfloatnullableW6825? Equivalent width of 6825 OVI0.1nmspect.line.eqWidthfloatnullableW7065? Equivalent width of 7065 HeI0.1nmspect.line.eqWidthfloatnullableJ/PAZh/41/148/table4The absolute intensities of the emission lines in the spectrum of V1329 CygrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJulian datedtime.epochintF4340? Absolute intensity of 4340 HImW.m**-2spect.line.intensity;em.line.HIdoublenullableF4471? Absolute intensity of 4471 HeImW.m**-2spect.line.intensitydoublenullableF4686? Absolute intensity of 4686 HeIImW.m**-2spect.line.intensitydoublenullableF4861? Absolute intensity of 4861 HImW.m**-2spect.line.intensity;em.line.HIdoublenullableF5319? Absolute intensity of 5319 FeIImW.m**-2spect.line.intensitydoublenullableF5412? Absolute intensity of 5412 HeIImW.m**-2spect.line.intensitydoublenullableF5616? Absolute intensity of 5616 [CaVII]mW.m**-2spect.line.intensitydoublenullableF5721? Absolute intensity of 5721 [FeVII]mW.m**-2spect.line.intensitydoublenullableF5876? Absolute intensity of 5876 HeImW.m**-2spect.line.intensitydoublenullableF6087? Absolute intensity of 6087 [FeVII]mW.m**-2spect.line.intensitydoublenullableF6375? Absolute intensity of 6375 [FeX]mW.m**-2spect.line.intensitydoublenullableF6563? Absolute intensity of 6563 HImW.m**-2spect.line.intensity;em.line.HIdoublenullableF6678? Absolute intensity of 6678 HeImW.m**-2spect.line.intensitydoublenullableF6825? Absolute intensity of 6825 OVImW.m**-2spect.line.intensitydoublenullableF7065? Absolute intensity of 7065 HeImW.m**-2spect.line.intensitydoublenullableJ/PAZh/41/148/table5Observed continuum fluxes from V1329 CygrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJulian datedtime.epochintFc4500? Observed continuum flux at 4500{AA} (mW/m2/{AA})10mW.m**-2.nm**-1phot.flux.density;spect.continuumdoublenullableFc6000? Observed continuum flux at 6000{AA} (mW/m2/{AA})10mW.m**-2.nm**-1phot.flux.density;spect.continuumdoublenullableFc7000? Observed continuum flux at 7000{AA} (mW/m2/{AA})10mW.m**-2.nm**-1phot.flux.density;spect.continuumdoublenullableJ/PAZh/41/148/table1UBV-observations of V1329 Cyg in 2003-2014recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJulian datedtime.epochintVmagV magnitudemagphot.mag;em.opt.VfloatBmagB magnitudemagphot.mag;em.opt.BfloatUmagU magnitudemagphot.mag;em.opt.UfloatB-VB-V color indexmagphot.color;em.opt.B;em.opt.VfloatU-BU-B color indexmagphot.color;em.opt.U;em.opt.Bfloat