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<ri:Resource created="2013-01-18T09:37:36Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>HI shells in Leiden/Argentina/Bonn HI survey</title><shortName>J/A+A/550/A23</shortName><identifier>ivo://CDS.VizieR/J/A+A/550/A23</identifier><altIdentifier>doi:10.26093/cds/vizier.35500023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ehlerova S.</name></creator><creator><name>Palous J.</name></creator><date role="Updated">2017-12-15T10:55:40Z</date><date role="Created">2013-01-18T09:37:36Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>milky-way-galaxy</subject><subject>interstellar-medium</subject><subject>h-i-line-emission</subject><description>We analyse the all-sky Leiden/Argentina/Bonn HI survey, where we identify shells belonging to the Milky Way. We used an identification method based on the search of continuous regions of a low brightness temperature that are compatible with given properties of HI shells. We found 333 shells in the whole Galaxy. The size distribution of shells in the outer Galaxy is fitted by a power law with the coefficient of 2.6 corresponding to the index 1.8 in the distribution of energy sources. Their surface density decreases exponentially with a scale length of 2.8kpc. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Seq</name><description>Sequential number, within the table</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name of the shell (LLL.l+BB.b+VVV.v)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType><flag>primary</flag></column><column><name>O</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>GLON1</name><description>Minimum galactic longitude of the shell</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLON2</name><description>Maximum galactic longitude of the shell</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT1</name><description>Minimum galactic latitude of the shell</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GLAT2</name><description>Maximum galactic latitude of the shell</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV1</name><description>Minimum radial velocity of the shell</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV2</name><description>Maximum radial velocity of the shell</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position of center, computed from the position in the name (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position of center, computed from the position in the name (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/A+A/550/A23/tablea2</name><description>Derived properties of HI shells in the outer Galaxy</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Seq</name><description>Sequential number, within the table</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name of the shell (LLL.l+BB.b+VVV.v)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>Rgc</name><description>Galactocentric distance of the shell</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad</name><description>Radius of the shell</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vexp</name><description>Expansion velocity of the shell</description><unit>km/s</unit><ucd>phys.veloc.expansion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L</name><description>Estimated energy input (the unit represent supernovae/million years)</description><unit>1e+44J.Myr**-1</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>texp</name><description>Estimated age</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>