J/AZh/88/380ivo://CDS.VizieR/J/AZh/88/380CDSRustamov D.N.Cherepashchuk A.M.2017-07-10T15:25:46Z2011-06-16T17:09:40ZCDS support team

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

cds-question@unistra.frvariable-starsspectroscopyline-intensitiesradial-velocityWe have used 46 high-resolution echelle spectra of the Wolf-Rayet star HD 192163 taken in 2005-2009 at the Cassegrain focus of the 2-m Zeiss-2000 telescope of the Shamakha Astrophysical Observatory to study profiles of the five strongest emission lines (HeII 4859, HeII 5411, CIV 5808, HeI 5875, (HeII+Halpha) 6560). We also obtained four echelle spectrograms of the Wolf-Rayet star HD 191765 for a comparative study of the NaI 5890 (D2) and NaI 5896 (D1) interstellar absorption lines. The echelle spectrograms were reduced using the DECH20 code. We determined the equivalent widths, radial velocities, central intensities, and half-widths of the emission lines. We We also studied the NaI 5890 (D2) and NaI 5896 (D1) interstellar absorption lines, which are important for understanding the nature of the nebula NGC 6888, whose origin is related to HD 192163.2011AZh....88..380Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/88/380CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/88/380https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/88/380http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/88/380https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/88/380https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/88/380http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AZh/88/380GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/AZh/88/380/WR136Combined table from original tablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintJDJulian datedtime.epochdoublePhasePhasetime.phasefloatWHe2aHeII 4859 equivalent width0.1nmspect.line.eqWidthfloatWHe2bHeII 5411 equivalent width0.1nmspect.line.eqWidthfloatWC4CIV 5808 equivalent width0.1nmspect.line.eqWidthfloatWHe1HeI 5875 equivalent width0.1nmspect.line.eqWidthfloatWHe2+HaHeII + H{alpha} equivalent width0.1nmspect.line.eqWidth;em.line.HalphafloatVHe2aHeII 4859 radial velocitykm/sspect.dopplerVelocfloatVHe2bHeII 5411 radial velocitykm/sspect.dopplerVelocfloatVC4CIV 5808 radial velocitykm/sspect.dopplerVelocfloatVHe1HeI 5875 radial velocitykm/sspect.dopplerVelocfloatVHe2+HaHeII + H{alpha} radial velocitykm/sspect.dopplerVelocfloatIHe2aHeII 4859 central intensityspect.line.intensityfloatwHe2aHeII 4859 half-width0.1nmspect.line.widthintIHe2bHeII 5411 central intensityspect.line.intensityfloatwHe2bHeII 5411 half-width0.1nmspect.line.widthintIC4CIV 5808 central intensityspect.line.intensityfloatwC4CIV 5808 half-width0.1nmspect.line.widthintIHe1HeI 5875 central intensityspect.line.intensityfloatwHe1HeI 5875 half-width0.1nmspect.line.widthintIHe2+HaHeII + H{alpha} central intensityspect.line.intensityfloatwHe2+HaHeII + H{alpha} half-width0.1nmspect.line.widthintWNa2NaI 5890 (D2) equivalent width from direct integration0.1nmspect.line.eqWidthfloatWNa2gNaI 5890 (D2) equivalent width from fitting Gaussian profiles0.1nmspect.line.eqWidthfloatWNa1NaI 5896 (D1) equivalent width from direct integration0.1nmspect.line.eqWidthfloatWNa1gNaI 5896 (D1) equivalent width from fitting Gaussian profiles0.1nmspect.line.eqWidthfloatVNa2Radial velocity of the NaI 5890 (D2) interstellar absorption linekm/sspect.dopplerVelocfloatVNa1Radial velocity of the NaI 5896 (D1) interstellar absorption linekm/sspect.dopplerVelocfloat