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<ri:Resource created="2021-08-12T09:40:24Z" 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>RGB abundances in the disk, stream &amp; halo of M31</title><shortName>J/ApJ/889/177</shortName><identifier>ivo://CDS.VizieR/J/ApJ/889/177</identifier><altIdentifier>doi:10.26093/cds/vizier.18890177</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Escala I.</name></creator><creator><name>Gilbert K.M.</name></creator><creator><name>Kirby E.N.</name></creator><creator><name>Wojno J.</name></creator><creator><name>Cunningham E.C.,Guhathakurta P.</name></creator><date role="Updated">2022-11-03T07:06:39Z</date><date role="Created">2021-08-12T09:40:24Z</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>galaxies</subject><subject>chemical-abundances</subject><subject>giant-stars</subject><subject>radial-velocity</subject><subject>halo-stars</subject><description>We measured [Fe/H] and [{alpha}/Fe] using spectral synthesis of low-resolution stellar spectroscopy for 70 individual red-giant-branch stars across four fields spanning the outer disk, Giant Stellar Stream (GSS), and inner halo of M31. Fields at M31-centric projected distances of 23kpc in the halo, 12kpc in the halo, 22kpc in the GSS, and 26kpc in the outer disk are {alpha}-enhanced, with &lt;[{alpha}/Fe]&gt;=0.43, 0.50, 0.41, and 0.58, respectively. The 23 and 12kpc halo fields are relatively metal-poor, with &lt;[Fe/H]&gt;=-1.54 and -1.30, whereas the 22kpc GSS and 26kpc outer disk fields are relatively metal-rich with &lt;[Fe/H]&gt;=-0.84 and -0.92, respectively. For fields with substructure, we separated the stellar populations into kinematically hot stellar halo components and kinematically cold components. We did not find any evidence of a radial [{alpha}/Fe] gradient along the high surface brightness core of the GSS between ~17 and 22kpc. However, we found tentative suggestions of a negative radial [{alpha}/Fe] gradient in the stellar halo, which may indicate that different progenitor(s) or formation mechanisms contributed to the build up of the inner versus outer halo. Additionally, the [{alpha}/Fe] distribution of the metal-rich ([Fe/H]&gt;-1.5), smooth inner stellar halo (r_proj_&lt;~26kpc) is inconsistent with having formed from the disruption of a progenitor(s) similar to present-day M31 satellite galaxies. The 26kpc outer disk is most likely associated with the extended disk of M31, where its high {alpha}-enhancement provides support for an episode of rapid star formation in M31's disk possibly induced by a major merger.</description><source format="bibcode">2020ApJ...889..177E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/889/177</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</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/433/185">J/A+A/433/185 : Abundance analysis of 102 F and G dwarfs (Bensby+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/367/1329">J/MNRAS/367/1329 : Elemental abundances for 176 stars (Reddy+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/183">J/MNRAS/383/183 : CaII triplet of RGB from VLT/FLAMES obs. 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