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<ri:Resource created="2018-12-18T15:30:21Z" 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>RRab stars of Monoceros Ring &amp; A13 overdensities</title><shortName>J/ApJ/854/47</shortName><identifier>ivo://CDS.VizieR/J/ApJ/854/47</identifier><altIdentifier>doi:10.26093/cds/vizier.18540047</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sheffield A.A.</name></creator><creator><name>Price-Whelan A.M.</name></creator><creator><name>Tzanidakis A.</name></creator><creator><name>Johnston K.V.,Laporte C.F.P.</name></creator><creator><name>Sesar B.</name></creator><date role="Updated">2019-01-09T08:07:24Z</date><date role="Created">2018-12-18T15:30:21Z</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>stellar-associations</subject><subject>variable-stars</subject><subject>radial-velocity</subject><subject>stellar-distance</subject><subject>visible-astronomy</subject><description>The Monoceros Ring (also known as the Galactic Anticenter Stellar Structure) and A13 are stellar overdensities at estimated heliocentric distances of d~11kpc and 15kpc observed at low Galactic latitudes toward the anticenter of our Galaxy. While these overdensities were initially thought to be remnants of a tidally disrupted satellite galaxy, an alternate scenario is that they are composed of stars from the Milky Way (MW) disk kicked out to their current location due to interactions between a satellite galaxy and the disk. To test this scenario, we study the stellar populations of the Monoceros Ring and A13 by measuring the number of RR Lyrae and M giant stars associated with these overdensities. We obtain low-resolution spectroscopy for RR Lyrae stars in the two structures and measure radial velocities to compare with previously measured velocities for M giant stars in the regions of the Monoceros Ring and A13, to assess the fraction of RR Lyrae to M giant stars (f_RR:MG_) in A13 and Mon/GASS. We perform velocity modeling on 153 RR Lyrae stars (116 in the Monoceros Ring and 37 in A13) and find that both structures have very low f_RR:MG_. The results support a scenario in which stars in A13 and Mon/GASS formed in the MW disk. We discuss a possible association between Mon/GASS, A13, and the Triangulum-Andromeda overdensity based on their similar velocity distributions and f_RR:MG_.</description><source format="bibcode">2018ApJ...854...47S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/854/47</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/317">I/317 : The PPMXL Catalog (Roeser+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1177">J/AJ/128/1177 : Galactic stellar abundances (Venn+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/442/1127">J/A+A/442/1127 : Library of 2500-10500{AA} synthetic spectra (Munari+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/717">J/ApJ/708/717 : Light curve templates of RR Lyrae stars (Sesar+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/146">J/ApJ/736/146 : Radial velocities of stars in Bootes I (Koposov+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/4">J/ApJ/731/4 : Galactic halo as seen by the CFHTLS (Sesar+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/114">J/AJ/144/114 : Radial velocities of 6 field RR Lyrae (Sesar+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/32">J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/776/26">J/ApJ/776/26 : RRab stars in the Orphan stream distances (Sesar+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/62">J/ApJ/793/62 : Triangulum-Andromeda stellar properties (Sheffield+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/L4">J/ApJ/844/L4 : PS1 RRab for tracing outer Virgo overdensity (Sesar+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/204">J/AJ/153/204 : RR Lyrae stars from the PS1 3{pi} survey (Sesar+, 2017)</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/ApJ/854/47</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/854/47</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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