J/AZh/74/63ivo://CDS.VizieR/J/AZh/74/63CDSMalov I.F.Malov O.I.2019-02-27T13:53:29Z1999-04-07T17:51:39ZCDS support team

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

cds-question@unistra.frpulsarsThe catalogue of pulsars with several calculated data is used by the cluster analysis for the division of pulsars into groups. Pulsars with periods P>1s and P<0.1s form two separate classes; the short-period objects, in turn, divide into two groups. One of these consist of young pulsars that form in the galactic plane or in globular clusters, while the other group consist of spun-up pulsars.1997AZh....74...63Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/74/63CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/74/63https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/74/63http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/74/63https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/74/63https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/74/63http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AZh/74/63GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapRadiodefaultJ/AZh/74/63/table1Pulsar cataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[001-218] Running numbermeta.id;meta.mainintPSRName of pulsarmeta.idcharPerPeriodstime.periodfloatPdotPeriod derivativefs/stime.perioddoublew50? Profile width at 50% of peakmsspect.line.widthdoublenullablelogLLog of integrated radio luminositylog(1e-07W)phys.luminosity;em.radiofloatlogBLog of magnetic field in gauss at the surfacelog(G)phys.magFieldfloatlogAgeLog of characteristic age in yearslog(yr)time.agefloat|z|Distance from the galactic planekpcpos.cartesian.z;pos.galacticfloatalf2? Spectral index of the linear part of pulsar spectrumspect.indexfloatnullablenumax? Frequency of the maximum of the spectrumGHzem.freq;stat.maxfloatnullablenucut? Frequency of the cutoff in the spectrumGHzmeta.notefloatnullablelogBlcMagnetic field in gauss at the light cylinderlog(G)phys.composition.massLightRatio;obs.fieldfloatbeta? Angle between rotation and magnetic axesdegphys.magField;pos.angDistancefloatnullableC? Maximum derivative of linear polarization position anglepos.posAng;phys.polarizationfloatnullablelogetaLog of efficiency of the transformation of rotation energy into radio emission (always negative)stat.paramfloat