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<ri:Resource created="2021-11-19T07:34:29Z" 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>FEDReD III: Unraveling the 3D structure of Vela</title><shortName>J/A+A/655/A68</shortName><identifier>ivo://CDS.VizieR/J/A+A/655/A68</identifier><altIdentifier>doi:10.26093/cds/vizier.36550068</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hottier C.</name></creator><creator><name>Babusiaux C.</name></creator><creator><name>Arenou F.</name></creator><date role="Updated">2022-03-10T07:24:47Z</date><date role="Created">2021-11-19T07:34:29Z</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>extinction</subject><subject>molecular-clouds</subject><description>The Vela complex is a region of the sky that gathers several stellar and interstellar structures in a few hundred square degrees. Gaia data now allows us to obtain a 3D view of the Vela interstellar structures through the dust extinction. We used the FEDReD (Field Extinction-Distance Relation Deconvolver) algorithm on near-infrared 2MASS data, cross-matched with the Gaia DR2 catalogue, to obtain a 3D cube of extinction density. We applied the FellWalker algorithm on this cube to locate clumps and dense structures. We analysed 18 million stars on 450 deg 2 to obtain the extinction density of the Vela complex from 0.5 to 8kpc at l in [250, 280] and b in [-10, 5].This cube reveals the complete morphology of known structures and relations between them. In particular, we show that the Vela Molecular Ridge is more likely composed by three substructures instead of four, as suggested by the 2D densities. These substructures form the shell of a large cavity. This cavity is visually aligned with the Vela supernova remnant but located at a larger distance. 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xsi:type="vs:VOTableType">double</dataType></column><column><name>maxb</name><description>[-4.81/0.34] Maximum b of edge</description><unit>deg</unit><ucd>pos.galactic.lat;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_maxb</name><description>[0.04/1.0] Standard deviation of maximum b of edge</description><unit>deg</unit><ucd>stat.stdev;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>minl</name><description>[255.3/277.31] Minimum l of edge</description><unit>deg</unit><ucd>pos.galactic.lon;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_minl</name><description>[0.0/3.06] Standard deviation of minimum l of edge</description><unit>deg</unit><ucd>stat.stdev;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>maxl</name><description>[257.99/278.02] Maximum l of 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xsi:type="vs:VOTableType">double</dataType></column><column><name>maxb</name><description>[-5.6/5.54] Maximum b of edge</description><unit>deg</unit><ucd>pos.galactic.lat;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_maxb</name><description>[0.0/1.11] Standard deviation of maximum b of edge</description><unit>deg</unit><ucd>stat.stdev;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>minl</name><description>[249.67/277.43] Minimum l of edge</description><unit>deg</unit><ucd>pos.galactic.lon;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_minl</name><description>[0/1.22] Standard deviation of minimum l of edge</description><unit>deg</unit><ucd>stat.stdev;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>maxl</name><description>[251.95/280.55] Maximum l of 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The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/A+A/655/A68/extdens</name><description>Extinction density (a0) cube flattened, original shape (77, 155, 208)</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column><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>GLAT</name><description>[-9.79/4.65] Barycentre Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><flag>indexed</flag></column><column><name>GLON</name><description>[250.38/279.64] Barycentre Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd><flag>indexed</flag></column><column><name>d</name><description>[0.2/24.27] Barycentre distance</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>a0</name><description>[-0.1/20.1]? Extinction density</description><unit>mag/kpc</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>s_a0</name><description>[0/1.9]? std of extinction density</description><unit>mag/kpc</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/A+A/655/A68/ext</name><description>Extinction (A0) cube flattened, original shape (77, 155, 209)</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>GLAT</name><description>[-9.79/4.65] Barycentre Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><flag>indexed</flag></column><column><name>GLON</name><description>[250.38/279.64] Barycentre Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd><flag>indexed</flag></column><column><name>d</name><description>[0.2/24.55] Barycentre distance</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>A0</name><description>[0/11.70]? Extinction</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0max</name><description>[0/19.96]? Maximum extinction</description><unit>mag</unit><ucd>phys.absorption;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0min</name><description>[0/10.61]? Minimum extinction</description><unit>mag</unit><ucd>phys.absorption;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table></schema></tableset></ri:Resource>