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<ri:Resource created="2022-09-19T09:18:09Z" 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>Galactic anticenter substructure stars from LAMOST</title><shortName>J/ApJ/910/46</shortName><identifier>ivo://CDS.VizieR/J/ApJ/910/46</identifier><altIdentifier>doi:10.26093/cds/vizier.19100046</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li J.</name></creator><creator><name>Xue X.-X.</name></creator><creator><name>Liu C.</name></creator><creator><name>Zhang B.</name></creator><creator><name>Rix H.-W.</name></creator><creator><name>Carlin J.L.</name></creator><creator><name>Yang C.,Mendez R.A.</name></creator><creator><name>Zhong J.</name></creator><creator><name>Tian H.</name></creator><creator><name>Zhang L.</name></creator><creator><name>Xu Y.</name></creator><creator><name>Wu Y.</name></creator><creator><name>Zhao G.</name></creator><creator><name>Chang R.</name></creator><date role="Updated">2022-09-30T23:19:25Z</date><date role="Created">2022-09-19T09:18:09Z</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>giant-stars</subject><subject>k-stars</subject><subject>proper-motions</subject><subject>radial-velocity</subject><subject>chemical-abundances</subject><subject>surveys</subject><subject>visible-astronomy</subject><description>We characterize the kinematic and chemical properties of 589 Galactic anticenter substructure stars (GASS) with K/M giants in integrals-of-motion space. These stars likely include members of previously identified substructures such as Monoceros, A13, and the Triangulum-Andromeda cloud. We show that these stars are in nearly circular orbits on both sides of the Galactic plane. We can see a velocity (VZ) gradient along Y-axis especially for the south GASS members. Our GASS members have similar energy and angular momentum distributions to thin-disk stars. Their location in [{alpha}/M] versus [M/H] space is more metal-poor than typical thin-disk stars, with [{alpha}/M] lower than that of the thick disk. We infer that our GASS members are part of the outer metal-poor disk stars and that the outer disk extends to 30 kpc. Considering the distance range and {alpha}-abundance features, GASS could be formed after the thick disk was formed due to the molecular cloud density decreasing in the outer disk where the star-formation rate might be less efficient compared to the inner disk.</description><source format="bibcode">2021ApJ...910...46L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/910/46</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/III/46">III/46 : Ap and Am Stars (Bertaud+ 1974; Bidelman+ 1973)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/100/1191">J/AJ/100/1191 : Giants DDO photometry (Morrison+, 1990)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/96/175">J/ApJS/96/175 : Kinematics of Metal-Poor Stars. 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