J/A+A/229/362ivo://CDS.VizieR/J/A+A/229/362doi:10.26093/cds/vizier.32290362CDSDeul E.R.den Hartog R.H.2018-02-12T08:45:34Z2010-09-13T13:11:27ZCDS support team

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

cds-question@unistra.frinterstellar-mediumh-i-line-emissiongalaxy-classification-systemsRecent high-resolution HI observations of M33 reveal a large number of regions that are devoid of emission. We interpret these regions as holes formed by interstellar winds; a catalogue containing 148 of these HI holes has been compiled. Their diameters range from the survey resolution limit (>40pc) to 1kpc. The swept-up mass, estimated from surrounding HI densities, ranges from 10^3^M_{sun}_ to 10^7^M_{sun}_. Energies needed to excavate such holes are between 10^49^ to 10^54^erg. Indicative ages, based on derived expansion velocities and diameters, show a cutoff near 7x10^6^yr. Three statistical analysis techniques are applied to determine positional correlation of the H I holes with H II regions, OB associations, and supernova remnants.1990A&A...229..362Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/229/362CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/229/362https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/229/362http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/229/362https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/229/362https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/229/362http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/229/362GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/229/362/table1 (Properties of the H I holes in the catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/229/362/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/229/362/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/229/362/table1?GETtext/xml+votable180.050000true23.1136230.439680.0055555555555555566/2154-2155 2240-2241https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/229/362?format=asciiOpticalRadiodefaultJ/A+A/229/362/table1Properties of the H I holes in the catalogueRAB1950Right ascension in decimal degrees (B1950)degpos.eq.ra;meta.mainrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[DD90]Sequential number of the holemeta.recordintprimaryDEB1950Declination in decimal degrees (B1950)degpos.eq.dec;meta.mainRDistance to the HI hole with respect to the M33 center (1)kpcpos.distancefloatthetaOrientation angle of the HI hole in the galaxy with respect to the north equatorial pole, with positive sense in the anti-clockwise directiondegpos.posAngfloatHRVRadial heliocentric velocity of maximum contrastkm/sspect.dopplerVeloc;stat.maxintDVExpansion velocity (to an accuracy of 2km/s)km/sphys.veloc.expansionintContHole contrast defined as Cont=I(surr)-I(50%)/I(surr)spect.line.intensity;arith.ratiofloatT[1/3] Type of Hole (in Fig.1 of paper): 1=gap, 2=shift, 3=depressionmeta.code.classintQQuality of detection (-1 met for the hole)meta.code.qual;instr.saturationintC[cp] complete/partial classification code (2)meta.code.classcharMinExtent of the minor axis of the ellipse that can be fitted to the 50% intensity contour of a holepcphys.sizeintMajExtent of the major axis of the ellipse that can be fitted to the 50% intensity contour of a holepcphys.sizeintDiamDiameter of the hole, Diam=(Min+Maj)^1/2^pcpos.distanceintepsEccentricity of the holesrc.orbital.eccentricityfloatPA[-90/90] Position angle of the major axis of the ellipse fitteddegpos.posAngintAgeKinematic age assuming a constant expansion velocityGyrtime.agefloatnHIAmbiant density derived from the observed total column densities for the HI material surrounding the holecm**-3phys.densityfloatMassMass assuming that nHi equals the pre-hole density and a spherical hole.10000solMassphys.massfloatEnergyEnergy needed to create the hole (x10^50^ergs)1e+43Jphys.energyfloat_RA.icrsRight ascension (ICRS) (computed by VizieR, not part of the original data)degpos.eq.ranullableindexed_DE.icrsDeclination (ICRS) (computed by VizieR, not part of the original data)degpos.eq.decnullableindexedJ/A+A/229/362/table2Overlap properties of the H I holes with respect to the H II regions and OB associationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[DD90]Sequential number of the holemeta.recordintHIIName of the HII region, CPSDP, Courtes et al., 1987, Cat. <J/A+AS/131/317>meta.notecharEM[1-4]? Emission measure code (1)meta.codeintnullableHI[1-3]? HI-HII code (2)meta.codeintnullableOB? OB association number, [HS80], Humphreys & Sandage, 1980ApJS...44..319Hmeta.id.associntnullableHI-OB[1-3]? HI-OB code (2)meta.codeintnullableHII-OB[1-3]? HII-OB code (2)meta.codeintnullable