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<ri:Resource created="2021-07-28T07:12:43Z" status="active" updated="2025-06-13T15:25:00Z" 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>Spiral arms Gaia EDR3</title><shortName>J/A+A/651/A104</shortName><identifier>ivo://CDS.VizieR/J/A+A/651/A104</identifier><altIdentifier>doi:10.26093/cds/vizier.36510104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Poggio E.</name></creator><creator><name>Drimmel R.</name></creator><creator><name>Cantat-Gaudin T.</name></creator><creator><name>Ramos P.</name></creator><creator><name>Ripepi V.</name></creator><creator><name>Zari E.,Andrae R.</name></creator><creator><name>Blomme R.</name></creator><creator><name>Chemin L.</name></creator><creator><name>Clementini G.</name></creator><creator><name>Figueras F.</name></creator><creator><name>Fouesneau M.,Fremat Y.</name></creator><creator><name>Lobel A.</name></creator><creator><name>Marshall D.J.</name></creator><creator><name>Muraveva T.</name></creator><creator><name>Romero-Gomez M.</name></creator><date role="Updated">2023-02-04T18:08:02Z</date><date role="Created">2021-07-28T07:12:43Z</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>open-star-clusters</subject><subject>proper-motions</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>Using the astrometry and integrated photometry from the Gaia Early Data Release 3 (EDR3), we map the density variations in the distribution of young Upper Main Sequence (UMS) stars, open clusters and classical Cepheids in the Galactic disk within several kiloparsecs of the Sun. Maps of relative over/under-dense regions for UMS stars in the Galactic disk are derived, using both bivariate kernel density estimators and wavelet transformations. The resulting overdensity maps exhibit large-scale arches, that extend in a clumpy but coherent way over the entire sampled volume, indicating the location of the spiral arms segments in the vicinity of the Sun. Peaks in the UMS overdensity are well-matched by the distribution of young and intrinsically bright open clusters. By applying a wavelet transformation to a sample of classical Cepheids, we find that their overdensities possibly extend the spiral arm segments on a larger scale (~10kpc from the Sun). While the resulting map based on the UMS sample is generally consistent with previous models of the Sagittarius-Carina spiral arm, the geometry of the arms in the III quadrant (galactic longitudes 180{deg}&lt;l&lt;270{deg}) differs significantly from many previous models. In particular we find that our maps favour a larger pitch angle for the Perseus arm, and that the Local Arm extends into the III quadrant at least 4kpc past the Sun's position, giving it a total length of at least 8kpc.</description><source format="bibcode">2021A&amp;A...651A.104P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/651/A104</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/640/A1">J/A+A/640/A1 : Portrait Galactic disc 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name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RA_ICRS</name><description>[] Mean right ascension of members (ICRS) at Ep=2015.5</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>e_pmRA*</name><description>? Sigma=1.4826*MAD where MAD is the median absolute deviation of pmRA*</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmDE</name><description>? Median proper motion along DE of members</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType><flag>nullable</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.ra</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>DE_ICRS</name><description>Mean declination of members (ICRS) at Ep=2015.5</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>GLON</name><description>Mean Galactic longitude of members</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Mean Galactic latitude of members</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r50</name><description>Radius containing half the members</description><unit>deg</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>agenn</name><description>? Age (logt) of the cluster (from Cantat-gaudin et al., 2020A&amp;A...640A...1C)</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dmnn</name><description>? Distance modulus of the cluster (from Cantat-gaudin et al., 2020A&amp;A...640A...1C)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>distpc</name><description>? Distance in parsecs (converted distance modulus)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmRA*</name><description>? Median proper motion along RA of members, pmRA*cosDE</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_pmDE</name><description>? Sigma=1.4826*MAD where MAD is the median absolute deviation of pmRDE</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>plx</name><description>? Median parallax of members</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_plx</name><description>? Sigma=1.4826*MAD where MAD is the median absolute deviation of plc</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>nbB0</name><description>Number of members brighter than absolute magnitude 0 in the G band</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nbB2</name><description>Number of members brighter than absolute magnitude 2 in the G band</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nbB4</name><description>Number of members brighter than absolute magnitude 4 in the G band</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>