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<ri:Resource created="2014-01-18T13:07:31Z" 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>Kinematics of bulge red clump stars</title><shortName>J/A+A/555/A91</shortName><identifier>ivo://CDS.VizieR/J/A+A/555/A91</identifier><altIdentifier>doi:10.26093/cds/vizier.35550091</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vasquez S.</name></creator><creator><name>Zoccali M.</name></creator><creator><name>Hill V.</name></creator><creator><name>Renzini A.</name></creator><creator><name>Gonzalez O.A.</name></creator><creator><name>Gardner E.,Debattista Victor P.</name></creator><creator><name>Robin A.C.</name></creator><creator><name>Rejkuba M.</name></creator><creator><name>Baffico M.</name></creator><creator><name>Monelli M.,Motta V.</name></creator><creator/><creator><name>Minniti D.</name></creator><date role="Updated">2014-01-18T13:19:54Z</date><date role="Created">2014-01-18T13:07:31Z</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>radial-velocity</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>giant-stars</subject><description>The Galactic bulge is X-shaped, caused by the two southern arms of the X both crossing the lines of sight, producing a double red clump (one bright and one faint) in the color magnitude diagram. In this paper the authors measure the radial velocities and proper motions for a sample of 454 individual bulge giant stars, roughly equally distributed between the two red clumps to determine how such a structure could be formed from bar instabilities. The radial velocity distribution of stars in the bright red clump, which traces the closer overdensity of bulge stars, shows an excess of stars moving towards the Sun. Similarly, an excess of stars receding from the Sun is seen in the more distant overdensity, which is traced by faint red clump stars. This can be explained by the presence of stars on elongated orbits, which are most likely streaming along the arms of the X-shaped bulge. Proper motions for these stars are consistent with qualitative predictions of dynamical models of peanut-shaped bulges. Surprisingly, stars on elongated orbits have preferentially metal-poor (subsolar) metallicities, while the metal rich ones, in both overdensities, are preferentially found in more axisymmetric orbits.</description><source format="bibcode">2013A&amp;A...555A..91V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/555/A91</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/II/270">II/270 : TCS-CAIN: NIR Survey of the Galactic plane (Cabrera-Lavers+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/421/3362">J/MNRAS/421/3362 : Kinematics of galactic red clump stars (Bilir+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/57">J/AJ/143/57 : New RVs from the spectroscopic survey BRAVA II (Kunder+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/546/A57">J/A+A/546/A57 : Spectroscopy of red giants in the Bulge (Uttenthaler+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A91">J/A+A/534/A91 : Galactic Bulge Valinhos Observatory Catalog (Teixeira+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A80">J/A+A/534/A80 : Metallicity of clump giants in Baade's window (Hill+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A54">J/A+A/530/A54 : Abundances of 650 bulge red giants (Gonzalez+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A40">J/A+A/527/A40 : Faint Galactic red clump stars (Saguner+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/732/108">J/ApJ/732/108 : Abundances of 92 giants in Plaut's window (Johnson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/61/83">J/AcA/61/83 : OGLE-III photometric maps of Galactic Bulge (Szymanski+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/522/A79">J/A+A/522/A79 : High-Galactic-latitude red clump stars (Valentini+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/721/L28">J/ApJ/721/L28 : Red clump stars in Galactic Bulge from OGLE-III (Nataf+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/691/1387">J/ApJ/691/1387 : Spectroscopy of the Galactic bar. 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