J/A+AS/108/611ivo://CDS.VizieR/J/A+AS/108/611CDSLASTENNET E.FREIRE FERRERO R.1998-02-21T09:18:43Z1998-02-21T10:17:40ZCDS support team

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

cds-question@unistra.frpeculiar-variable-starsemission-line-stars(no description available)1994A&AS..108..611Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/108/611CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/108/611https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/108/611http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/108/611https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/108/611https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/108/611http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/108/611GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+AS/108/611/ca2Ca II K linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNoRunning numbermeta.idintHDstar's identification given by its HD number (except for some particular case like the `Sun', identified by its name)meta.id;meta.maincharSpSpectral typesrc.spTypecharClClass of luminositysrc.class.luminositycharMv[]? Absolute magnitude, as provided in the papers we consideredmagphys.magAbs;em.optfloatnullablelog(W)[]? Decimal logarithm of the line width (emission line core; data provided only by the papers studied) (1)log(km.s**-1)spect.line.widthfloatnullableRefReferences (2)meta.refintVmag[]? Visual magnitudemagphot.mag;em.opt.VfloatnullableB-V[]? B-V colourmagphot.color;em.opt.B;em.opt.VfloatnullableU-B[]? U-B colourmagphot.color;em.opt.U;em.opt.Bfloatnullablevsini[]? Rotational velocitykm/sphys.veloc.rotatfloatnullableremRemark V : variable star SB : spectroscopic binary e : emission star p : peculiar star CO : compagnonmeta.notecharplx91[]? Weigthed average absolute parallaxarcsecpos.parallax.trigfloatnullablee_plx91[]? rms uncertainty on plx91arcsecstat.errorfloatnullableN[]? Number of parallax observations included in weigthed average parallaxmeta.numberintnullableq_plx91[GFP ] Quality of the interagreement of different parallaxes observations (G = good, F = fair, P = poor)meta.code.qualcharn_Binar[BWOS ] Binarity of the collected stars when no number in the Aitken's catalog (3)meta.notecharBinar[]? Binarity of the collected stars. Nunber in the Aitken's catalog (ADS Catalog)meta.idintnullableV91[]? Visual magnitudemagphot.mag;em.opt.VfloatnullableMabs91[]? Absolute magnitude computed from the columns Plx91 and V91magphys.magAbs;em.optfloatnullablee_Mabs91[]? rms uncertainty on Mabs91. This column is computed from the columns Plx91 and e_Plx91magstat.errorfloatnullablerel-e_Plx91[]? Relative error on the parallaxes given by the columns Plx91 and e_Plx91arcsecstat.errordoublenullableJ/A+AS/108/611/ca2kCa II K lines: Kuhi data (Kuhi L.V., 1965, 1965PASP...77..253K)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNoRunning numbermeta.idintHDstar's identification given by its HD number (except for some particular case like the `Sun', identified by its name)meta.id;meta.maincharSpSpectral typesrc.spTypecharClClass of luminositysrc.class.luminositycharMv[]? Absolute magnitude, as provided in the papers we consideredmagphys.magAbs;em.optfloatnullablelog(W)[]? Decimal logarithm of the line width (emission line core; data provided only by the papers studied) (1)log(km.s**-1)spect.line.widthfloatnullableRefReferences (2)meta.refintVmag[]? Visual magnitudemagphot.mag;em.opt.VfloatnullableB-V[]? B-V colourmagphot.color;em.opt.B;em.opt.VfloatnullableU-B[]? U-B colourmagphot.color;em.opt.U;em.opt.Bfloatnullablevsini[]? Rotational velocitykm/sphys.veloc.rotatfloatnullableremRemark V : variable star SB : spectroscopic binary e : emission star p : peculiar star CO : compagnonmeta.notecharplx91[]? Weigthed average absolute parallaxarcsecpos.parallax.trigfloatnullablee_plx91[]? rms uncertainty on plx91arcsecstat.errorfloatnullableN[]? Number of parallax observations included in weigthed average parallaxmeta.numberintnullableq_plx91[GFP ] Quality of the interagreement of different parallaxes observations (G = good, F = fair, P = poor)meta.code.qualcharn_Binar[BWOS ] Binarity of the collected stars when no number in the Aitken's catalog (3)meta.notecharBinar[]? Binarity of the collected stars. Nunber in the Aitken's catalog (ADS Catalog)meta.idintnullableV91[]? Visual magnitudemagphot.mag;em.opt.VfloatnullableMabs91[]? Absolute magnitude computed from the columns Plx91 and V91magphys.magAbs;em.optfloatnullablee_Mabs91[]? rms uncertainty on Mabs91. This column is computed from the columns Plx91 and e_Plx91magstat.errorfloatnullablerel-e_Plx91[]? Relative error on the parallaxes given by the columns Plx91 and e_Plx91arcsecstat.errordoublenullableJ/A+AS/108/611/mg2Mg II k lineSpSpectral typesrc.spTypecharClClass of luminositysrc.class.luminositychare_plx91[]? rms uncertainty on plx91arcsecstat.errorfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNoRunning numbermeta.idintHDstar's identification given by its HD number (except for some particular case like the `Sun', identified by its name)meta.id;meta.maincharMv[]? Absolute magnitude, as provided in the papers we consideredmagphys.magAbs;em.optfloatnullablelog(W)[]? Decimal logarithm of the line width (emission line core; data provided only by the papers studied) (1)log(km.s**-1)spect.line.widthfloatnullableRefReferences (2)meta.refintVmag[]? Visual magnitudemagphot.mag;em.opt.VfloatnullableB-V[]? B-V colourmagphot.color;em.opt.B;em.opt.VfloatnullableU-B[]? U-B colourmagphot.color;em.opt.U;em.opt.Bfloatnullablevsini[]? Rotational velocitykm/sphys.veloc.rotatfloatnullableremRemark V : variable star SB : spectroscopic binary e : emission star p : peculiar star CO : compagnonmeta.notecharplx91[]? Weigthed average absolute parallaxarcsecpos.parallax.trigfloatnullableN[]? Number of parallax observations included in weigthed average parallaxmeta.numberintnullableq_plx91[GFP ] Quality of the interagreement of different parallaxes observations (G = good, F = fair, P = poor)meta.code.qualcharn_Binar[BWOS ] Binarity of the collected stars when no number in the Aitken's catalog (3)meta.notecharBinar[]? Binarity of the collected stars. Nunber in the Aitken's catalog (ADS Catalog)meta.idintnullableV91[]? Visual magnitudemagphot.mag;em.opt.VfloatnullableMabs91[]? Absolute magnitude computed from the columns Plx91 and V91magphys.magAbs;em.optfloatnullablee_Mabs91[]? rms uncertainty on Mabs91. This column is computed from the columns Plx91 and e_Plx91magstat.errorfloatnullablerel-e_Plx91[]? Relative error on the parallaxes given by the columns Plx91 and e_Plx91arcsecstat.errordoublenullableJ/A+AS/108/611/table5Bibliographical sources for the Ca II k linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNrefReference numbermeta.refintTypeType of measuresmeta.code;obscharRefReferencesmeta.refcharN[]? Number of distinct datameta.numberintnullableICorrInstrument correctioninstr.paramcharJ/A+AS/108/611/table6Bibliographical sources for the Mg II K linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNrefReference numbermeta.refintTypeType of measuresmeta.code;obscharRefReferencesmeta.refcharComCommentsmeta.notecharN[]? Number of distinct datameta.numberintnullablen_ICorr[n] n = no correctionmeta.notecharICorr[]? Instrument correction0.1nminstr.paramfloatnullable