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<ri:Resource created="2005-08-12T06:29:33Z" 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>Abundances in Milky Way's disk</title><shortName>J/A+A/438/139</shortName><identifier>ivo://CDS.VizieR/J/A+A/438/139</identifier><altIdentifier>doi:10.26093/cds/vizier.34380139</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Soubiran C.</name></creator><creator><name>Girard P.</name></creator><date role="Updated">2018-01-05T08:56:51Z</date><date role="Created">2005-08-12T06:29:33Z</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>chemically-peculiar-stars</subject><description>We have compiled a large catalogue of metallicities and abundance ratios from the literature in order to investigate abundance trends of several alpha and iron peak elements in the thin disk and the thick disk of the Galaxy. The catalogue includes 743 stars with abundances of Fe, O, Mg, Ca, Ti, Si, Na, Ni and Al in the metallicity range -1.30&lt;[Fe/H]&lt;+0.50. We have checked that systematic differences between abundances measured in the different studies were lower than random errors before combining them. Accurate distances and proper motions from Hipparcos, and radial velocities from several sources have been retrieved for 639 stars and their velocities (U,V,W) and galactic orbits have been computed. Ages of 322 stars have been estimated with the Bayesian method of isochrone fitting developed by Pont &amp; Eyer (2004MNRAS.351..487P). Two samples kinematically representative of the thin and thick disks have been selected, taking into account the Hercules stream which is intermediate in kinematics, but with a probable dynamical origin. Our results show that the two disks are chemically well separated, they overlap greatly in metallicity and both show parallel decreasing trends of alpha elements with increasing metallicity, in the interval -0.80&lt;[Fe/H]&lt;-0.30. The Mg enhancement with respect to Fe of the thick disk is measured to be 0.14dex. An even larger enhancement is observed for Al. The thick disk is clearly older than the thin disk with a tentative evidence of an AMR over 2-3Gyr and a hiatus in star formation before the formation of the thin disk. We do not observe a vertical gradient in the metallicity of the thick disk. The Hercules stream have properties similar to that of the thin disk, with a wider range of metallicity. Metal-rich stars assigned to the thick disk and super metal rich stars assigned to the thin disk appear as outliers in all their properties.</description><source format="bibcode">2005A&amp;A...438..139S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/438/139</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/A+A/438/139</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Sodium abundance relative to iron</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Mg/Fe]</name><description>? Magnesium abundance relative to iron</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Al/Fe]</name><description>? Aluminium abundance relative to iron</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Si/Fe]</name><description>Silicon abundance relative to iron</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ca/Fe]</name><description>? Calcium abundance relative to iron</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ti/Fe]</name><description>? Titanium abundance relative to iron</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ni/Fe]</name><description>? Nickel abundance relative to iron</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Uvel</name><description>? Galactic radial velocity (1)</description><unit>km/s</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vvel</name><description>? Galactic rotational velocity (1)</description><unit>km/s</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Wvel</name><description>? Galactic vertical velocity (1)</description><unit>km/s</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rmin</name><description>? Perigalactic distance</description><unit>kpc</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rmax</name><description>? Apogalactic distance</description><unit>kpc</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Zmax</name><description>? Maximum distance from galactic plane</description><unit>kpc</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ecc</name><description>? Eccentricity of galactic orbit</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>age</name><description>? Age, in Gigayears</description><unit>Gyr</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_age</name><description>? Relative error on age</description><unit>%</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pthin</name><description>? Thin disk membership probability</description><unit>%</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pthick</name><description>? Thick disk membership probability</description><unit>%</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PHer</name><description>? Hercules stream membership probability</description><unit>%</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Teff</name><description>Effective temperature</description><unit>K</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[alpha/Fe]</name><description>Mean alpha abundance (1)</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_VMAG</name><description>? One sigma lower limit of Mv (2)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_VMAG</name><description>? 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