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<ri:Resource created="2023-08-30T16:31:46Z" status="active" updated="2026-03-04T20:03:00Z" 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>Galactic classical Cepheids catalog</title><shortName>J/other/NatAs/3.</shortName><identifier>ivo://CDS.VizieR/J/other/NatAs/3.320</identifier><altIdentifier>doi:10.26093/cds/vizier/dt/dkdca</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen X.</name></creator><creator><name>Wang S.</name></creator><creator><name>Deng L.</name></creator><creator><name>De Grijs R.</name></creator><creator><name>Liu C.</name></creator><creator><name>Tian H.</name></creator><date role="Updated">2026-03-04T20:03:00Z</date><date role="Created">2023-08-30T16:31:46Z</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>variable-stars</subject><subject>infrared-photometry</subject><subject>stellar-distance</subject><subject>proper-motions</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>The Milky Way's neutral hydrogen (HI) disk is warped and flared. However, a dearth of accurate HI-based distances has thus far prevented the development of an accurate Galactic Disk model. Moreover, the extent to which our Galaxy's stellar and gas disk morphologies are mutually consistent is also unclear. Classical Cepheids, primary distance indicators with distance accuracies of 3-5%, offer a unique opportunity to develop an intuitive and accurate three-dimensional picture. Here, we establish a robust Galactic Disk model based on 1339 classical Cepheids. We provide strong evidence that the warp's line of nodes is not oriented in the Galactic Centre-Sun direction. Instead, it subtends a mean angle of 17.5{deg}+/-1{deg} (formal)+/-3{deg} (systematic) and exhibits a leading spiral pattern. Our Galaxy thus follows Briggs' rule for spiral galaxies, which suggests that the origin of the warp is associated with torques forced by the massive inner disk. The stellar disk traced by Cepheids follows the gas disk in terms of their amplitudes; the stellar disk extends to at least 20kpc. This morphology provides a crucial, updated map for studies of the kinematics and archaeology of the Galactic Disk.</description><source format="bibcode">2019NatAs...3..320C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/NatAs/3.320</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></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/NatAs/3.320</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/NatAs/3.320</mirrorURL><mirrorURL 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J/other/NatAs/3.320/tabled1 (Cepheid catalogue used in the research)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/other/NatAs/3.320/tabled1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/other/NatAs/3.320/tabled1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/other/NatAs/3.320/tabled1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>303.2266427</ra><dec>32.7011507</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>4/2333 5/763 907 3580 3603 3607 3650 3661 3842 3853 3863 3908 5905 9341 9430 9437 9455 9474-9475 9480-9482 9841 9854 10754-10755 6/336 1139 1239 1282 1290 1292 1296 1323 1326 1329 1331-1332 1340 1348 1358 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