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<ri:Resource created="2021-01-26T13:24:13Z" 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>Spectroscopic obs. of RR Lyrae in NGC5139</title><shortName>J/ApJ/881/104</shortName><identifier>ivo://CDS.VizieR/J/ApJ/881/104</identifier><altIdentifier>doi:10.26093/cds/vizier.18810104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Magurno+</name></creator><creator><name>Magurno D.</name></creator><creator><name>Sneden C.</name></creator><creator><name>Bono G.</name></creator><creator><name>Braga V.F.</name></creator><creator><name>Mateo M.,Persson S.E.</name></creator><creator><name>Preston G.</name></creator><creator><name>Thevenin F.</name></creator><creator><name>da Silva R.</name></creator><creator><name>Dall'Ora M.,Fabrizio M.</name></creator><creator><name>Ferraro I.</name></creator><creator><name>Fiorentino G.</name></creator><creator><name>Iannicola G.</name></creator><creator><name>Inno L.</name></creator><creator><name>Marengo M.,Marinoni S.</name></creator><creator><name>Marrese P.M.</name></creator><creator><name>Martinez-Vazquez C.E.</name></creator><creator><name>Matsunaga N.</name></creator><creator><name>Monelli M.,Neeley J.R.</name></creator><creator><name>Nonino M.</name></creator><creator><name>Walker A.R.</name></creator><date role="Updated">2022-06-03T08:24:07Z</date><date role="Created">2021-01-26T13:24:13Z</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>globular-star-clusters</subject><subject>variable-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>metallicity</subject><subject>radial-velocity</subject><description>We present a detailed spectroscopic analysis of RR Lyrae (RRL) variables in the globular cluster NGC5139 ({omega} Cen). We collected optical (4580-5330{AA}), high-resolution (R~34000), high signal-to-noise ratio (~200) spectra for 113 RRLs with the multifiber spectrograph M2FS at the Magellan/Clay Telescope at Las Campanas Observatory. We also analyzed high- resolution (R~26000) spectra for 122 RRLs collected with FLAMES/GIRAFFE at the Very Large Telescope, available in the ESO archive. The current sample doubles the literature abundances of cluster and field RRLs in the Milky Way based on high-resolution spectra. Equivalent-width measurements were used to estimate atmospheric parameters, iron, and abundance ratios for {alpha} (Mg, Ca, Ti), iron peak (Sc, Cr, Ni, Zn), and s-process (Y) elements. We confirm that {omega}Cen is a complex cluster, characterized by a large spread in the iron content: -2.58&lt;~[Fe/H]&lt;~-0.85. We estimated the average cluster abundance as &lt;[Fe/H]&gt;=-1.80{+/-}0.03, with {sigma}=0.33dex. Our findings also suggest that two different RRL populations coexist in the cluster. The former is more metal-poor ([Fe/H]&lt;~-1.5), with almost solar abundance of Y. The latter is less numerous, more metal-rich, and yttrium enhanced ([Y/Fe]&gt;~0.4). This peculiar bimodal enrichment only shows up in the s-process element, and it is not observed among lighter elements, whose [X/Fe] ratios are typical for Galactic globular clusters.</description><source format="bibcode">2019ApJ...881..104M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/881/104</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/J/AJ/110/2319">J/AJ/110/2319 : Abundances in RR Lyr variables (Clementini+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/462/241">J/ApJ/462/241 : Ca abundance for Omega Cen red giants (Norris+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/119/1824">J/AJ/119/1824 : Caby photometry of {Omega} Centauri (Rey+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/424/1101">J/A+A/424/1101 : Variable Stars in the field of {omega} Cen (Kaluzny+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/2140">J/AJ/130/2140 : Abundances and velocities globular clusters (Pritzl+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/370/1979">J/MNRAS/370/1979 : JHKs photometry of T2Cs globular clusters (Matsunaga+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/503">J/A+A/445/503 : Radial velocities in Omega Cen (NGC5139) (Reijns+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/640/L43">J/ApJ/640/L43 : Metallicities of RR Lyrae stars in Omega Cen (Sollima+,2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/1021">J/ApJ/663/1021 : Log of {omega} Cen scientific images (Castellani+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/667/1267">J/ApJ/667/1267 : CrI transition probabilities (Sobeck+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1447">J/AJ/133/1447 : Light curves of variable stars {omega}Cen (Weldrake+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/506">J/AJ/136/506 : Radial velocities {omega}Centauri members (Da Costa+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/706/1277">J/ApJ/706/1277 : Stromgren photometry in {omega} Cen (Calamida+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/139">J/A+A/505/139 : Abund. red giants in 17 globular clusters (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/121/1378">J/PASP/121/1378 : Positions variable stars in globular clusters (Samus+, 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/AJ/140/1694">J/AJ/140/1694 : Abundances of non-variable red and 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/ApJ/722/1373">J/ApJ/722/1373 : {omega} Centauri giants abundances (Johnson+, 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/ApJS/197/29">J/ApJS/197/29 : Chemical compositions of 11 RR Lyrae (For+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/64">J/ApJ/731/64 : Spectroscopy of 300 RGBs in {omega} Cen (Marino+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A53">J/A+A/534/A53 : Equivalent widths of 18 subgiant {omega}Cen (Pancino+, 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/751/102">J/ApJ/751/102 : Equivalent widths of 9 RGB in Carina dSph (Venn+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/27">J/ApJS/208/27 : Sun and HD 84937 TiII log(gf) and abundances (Wood+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/23">J/ApJS/215/23 : FeI radiative lifetime &amp; branching fract. 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Observing phase</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Type</name><description>Pulsation category; 44 RRab, 68 RRc or 1 RRd (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>f_Type</name><description>[*] Asterisk marks Blazhko RRLs (19 occurrences)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Vmag</name><description>[14.05/14.83] 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>[0.04/1.27] V band amplitude</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVel</name><description>[173/264] Radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FeH</name><description>Iron abundance for this star (link to table 6)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Abund</name><description>Other abundance for this star (link to table 8)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/881/104/table6</name><description>Iron abundances for the considered samples of {omega}Cen RR Lyrae.</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType><flag>nullable</flag></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>ID</name><description>Star identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>[Fe/H]EW</name><description>[-2.53/-0.85]? The [Fe/H] for M2FS with EW method</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]EW</name><description>[0.01/0.15]? Uncertainty in [Fe/H]EW</description><ucd>stat.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]PAP</name><description>[-2.58/-1.34]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>Star identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>[Mg/Fe]</name><description>[-0.07/0.95]? The [Mg/Fe] abundance ratio</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Mg/Fe]</name><description>[0.03/0.28]? Uncertainty in [Mg/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/Fe]</name><description>[0.17/0.63]? The [Ca/Fe] abundance ratio</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Ca/Fe]</name><description>[0.1/0.1]? 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Uncertainty in [a/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Sc/Fe]</name><description>[-0.4/0.66]? The [Sc/Fe] abundance ratio</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Sc/Fe]</name><description>[0.0/0.22]? Uncertainty in [Sc/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Cr/Fe]</name><description>[-0.34/0.57]? The [Cr/Fe] abundance ratio</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Cr/Fe]</name><description>[0.02/0.15]? Uncertainty in [Cr/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ni/Fe]</name><description>[-0.34/0.33]? The [Ni/Fe] abundance ratio</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Ni/Fe]</name><description>[0.03/0.2]? Uncertainty in [Ni/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Zn/Fe]</name><description>[0.1/0.41]? The [Zn/Fe] abundance ratio</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Zn/Fe]</name><description>[0.01/0.16]? Uncertainty in [Zn/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Y/Fe]</name><description>[-0.21/1.11]? The [Y/Fe] abundance ratio</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Y/Fe]</name><description>[0.0/0.21]? Uncertainty in [Y/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/881/104/table2</name><description>Line list and atomic parameters</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>[4589/5326] Wavelength ({AA})</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Species</name><description>Species identifier (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>ExPot</name><description>[0/4.4] Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf</name><description>[-4.12/0.57] log oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>