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<ri:Resource created="2022-12-23T10:10:24Z" 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>Field RR Lyrae as Gal. probes. III. Abundances</title><shortName>J/ApJ/914/10</shortName><identifier>ivo://CDS.VizieR/J/ApJ/914/10</identifier><altIdentifier>doi:10.26093/cds/vizier.19140010</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Crestani J.</name></creator><creator><name>Braga V.F.</name></creator><creator><name>Fabrizio M.</name></creator><creator><name>Bono G.</name></creator><creator><name>Sneden C.</name></creator><creator><name>Preston G.,Ferraro I.</name></creator><creator><name>Iannicola G.</name></creator><creator><name>Nonino M.</name></creator><creator><name>Fiorentino G.</name></creator><creator><name>Thevenin F.</name></creator><creator><name>Lemasle B.,Prudil Z.</name></creator><creator><name>Alves-Brito A.</name></creator><creator><name>Altavilla G.</name></creator><creator><name>Chaboyer B.</name></creator><creator><name>Dall'Ora M.,D'Orazi V.</name></creator><creator><name>Gilligan C.</name></creator><creator><name>Grebel E.K.</name></creator><creator><name>Koch-Hansen A.J.</name></creator><creator><name>Lala H.</name></creator><creator><name>Marengo M.,Marinoni S.</name></creator><creator><name>Marrese P.M.</name></creator><creator><name>Martinez-Vazquez C.</name></creator><creator><name>Matsunaga N.</name></creator><creator><name>Monelli M.,Mullen J.P.</name></creator><creator><name>Neeley J.</name></creator><creator><name>da Silva R.</name></creator><creator><name>Stetson P.B.</name></creator><creator><name>Salaris M.</name></creator><creator><name>Storm J.,Valenti E.</name></creator><creator><name>Zoccali M.</name></creator><date role="Updated">2025-02-13T20:11:22Z</date><date role="Created">2022-12-23T10:10:24Z</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>chemical-abundances</subject><subject>variable-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We provide the largest and most homogeneous sample of {alpha}-element (Mg, Ca, Ti) and iron abundances for field RR Lyrae (RRLs; 162 variables) by using high-resolution spectra. The current measurements were complemented with similar abundances available in the literature for 46 field RRLs brought to our metallicity scale. We ended up with a sample of old (t&gt;=10Gyr), low-mass stellar tracers (208 RRLs: 169 fundamental, 38 first overtone, and 1 mixed mode) covering 3dex in iron abundance (-3.00&lt;=[Fe/H]&lt;=0.24). We found that field RRLs are ~0.3dex more {alpha} poor than typical halo tracers in the metal-rich regime ([Fe/H]&gt;=-1.2), while in the metal-poor regime ([Fe/H]&lt;=-2.2) they seem to be on average ~0.1dex more {alpha} enhanced. This is the first time that the depletion in {alpha} elements for solar iron abundances is detected on the basis of a large, homogeneous, and coeval sample of old stellar tracers. Interestingly, we also detected a close similarity in the [{alpha}/Fe] trend between {alpha}-poor, metal-rich RRLs and red giants (RGs) in the Sagittarius dwarf galaxy as well as between {alpha}-enhanced, metal-poor RRLs and RGs in ultrafaint dwarf galaxies. These results are supported by similar elemental abundances for 46 field horizontal branch stars. These stars share with RRLs the same evolutionary phase and the same progenitors. This evidence further supports the key role that old stellar tracers play in constraining the early chemical enrichment of the halo and, in particular, in investigating the impact that dwarf galaxies have had in the mass assembly of the Galaxy.</description><source format="bibcode">2021ApJ...914...10C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/914/10</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/VII/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/110/2319">J/AJ/110/2319 : Abundances in RR Lyr variables (Clementini+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/340/304">J/MNRAS/340/304 : [X/Fe] of Galactic disc F and G dwarfs (Reddy+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/1117">J/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004)</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/AJ/130/2140">J/AJ/130/2140 : Abundances &amp; velocities in globular clusters (Pritzl+, 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/A+A/465/815">J/A+A/465/815 : Abundances of Sgr dSph stars (Sbordone+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/1580">J/AJ/135/1580 : Abundances in 10 red giants of Car dSph (Koch+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/139">J/A+A/505/139 : Abundances of red giants in 17 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/117">J/A+A/505/117 : Abundances of red giants in 15 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/1053">J/ApJ/701/1053 : Abundances of 8 stars in the Draco dSph (Cohen+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/712/L21">J/ApJ/712/L21 : Calcium abundances in 17 globular clusters (Carretta+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/520/A95">J/A+A/520/A95 : Abundances of red giants in M54 &amp; Sgr dSph (Carretta+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/1694">J/AJ/140/1694 : Abundances of non-variable red &amp; blue HB stars (For+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/331/474">J/AN/331/474 : Abundances of metal-poor stars (Frebel, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/560">J/ApJ/708/560 : Spectroscopy of UMa II and Coma Ber (Frebel+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A17">J/A+A/523/A17 : Individual stars in Fornax dSph center (Letarte+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/L10">J/A+A/511/L10 : Abundances and space velocities of 94 stars (Nissen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/A56">J/A+A/511/A56 : Abundances of five open clusters (Pancino+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/29">J/ApJS/197/29 : Chemical compositions of 11 RR Lyrae (For+, 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/ApJ/778/149">J/ApJ/778/149 : Abundances for 3 stars in Sgr dSph (McWilliam+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/134">J/ApJ/767/134 : Abundances of red giant stars in UFD gal. 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Uncertainty in [Ti/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[a/Fe]</name><description>[-0.2/0.71] Median Solar-scaled {alpha}-element abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>e_[a/Fe]</name><description>[0/0.23] Uncertainty in [alpha/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sample</name><description>Sample ("Lit-HB", "Lit-RRL" or "TW-RRL"=this work RRL)</description><ucd>src.sample</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Ref</name><description>Source (1)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>PapII</name><description>Display data from Paper II (Crestani+ 2021, J/ApJ/908/20)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>S</name><description>Display the basic information for this RRL (link to Table 2)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Nab</name><description>Number of measurements derived in this work for this RRL (link to Table 4)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>A</name><description>Display the abundances adopted from the literature for this RRL (link to Table 3)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/914/10/table2</name><description>Basic information of the entire RR Lyrae sample</description><column><name>GaiaDR2</name><description>Gaia DR2 identification</description><ucd>meta.id;meta.main</ucd></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>OName</name><description>Other name for the star</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Epoch=2015.5</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>[-84.41/69.52] Declination (ICRS) at Epoch=2015.5</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Vmag</name><description>[7.78/17.24] Mean V-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vamp</name><description>[0.25/1.31] V-band amplitude</description><unit>mag</unit><ucd>src.var.amplitude;phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>[0.2/0.81] Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Class</name><description>Pulsation mode ("RRab", "RRc" or "RRd")</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Sample</name><description>Sample ("Lit-RRL" or "TW-RRL"=this work; 162 occurrences)</description><ucd>src.sample</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table><table><name>J/ApJ/914/10/table3</name><description>RRL abundances adopted from the literature</description><column><name>GaiaDR2</name><description>Gaia DR2 identification</description><ucd>meta.id;meta.main</ucd></column><column><name>[Mg/Fe]o</name><description>[0.21/0.63]? Solar-scaled magnesium abundance in the literature source (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/Fe]o</name><description>[-0.11/0.52]? Solar-scaled calcium abundance in the literature source (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ti/Fe]o</name><description>[0.18/0.8]? Solar-scaled titanium abundance in the literature source (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ref</name><description>Literature source (2)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Fe/H]o</name><description>[-2.9/-0.21] Solar-scaled metallicity in the literature source (1)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-2.83/-0.21] Solar-scaled metallicity transformed to our scale (1)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Mg/Fe]</name><description>[0/0.6]? Solar-scaled magnesium abundance transformed to our scale (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/Fe]</name><description>[-0/0.54]? Solar-scaled calcium abundance transformed to our scale (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ti/Fe]</name><description>[0.28/0.91]? Solar-scaled titanium abundance transformed to our scale (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/914/10/table4</name><description>Atmospheric parameters derived in this work for each individual measurement</description><column><name>GaiaDR2</name><description>Gaia DR2 identification</description><ucd>meta.id;meta.main</ucd></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Inst</name><description>Spectrograph identification</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Teff</name><description>[5750/8220] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[0/940] Uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(g)</name><description>[0.79/4] Log, Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(g)</name><description>[0.04/0.42] Uncertainty in log (g)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt</name><description>[1.19/5.82] Microturbulent velocity, {xi}_t_</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vt</name><description>[0.05/2.5] Uncertainty in Vt</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[FeI/H]</name><description>[-3.11/0.23] Median Solar-scaled iron abundance of neutral iron lines</description><ucd>phys.abund.Fe;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeI/H]</name><description>[0.06/0.28] Uncertainty in [FeI/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NFeI</name><description>[9/234] Number of adopted neutral iron lines</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[FeII/H]</name><description>[-3.11/0.23] Median Solar-scaled iron abundance of singly ionized iron lines</description><ucd>phys.abund.Fe;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeII/H]</name><description>[0.01/0.83] Uncertainty [FeII/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NFeII</name><description>[2/39] Number of adopted singly ionized iron line</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nstack</name><description>[1/8] Number of individual spectra stacked for this measurement</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/ApJ/914/10/table5</name><description>List of {alpha}-element transitions adopted in this work</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>[3729.81/8717.83] Vacuum wavelength</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ion</name><description>[12/22.1] Species</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EP</name><description>[0/5.932] Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>[-5.62/0.57] log, statistical weight*oscillator strength</description><ucd>stat.weight;phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref</name><description>Line parameters reference (1)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table></schema></tableset></ri:Resource>