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<ri:Resource created="2018-03-28T10:38:21Z" 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>RRLs in globulars. IV. UBVRI photometry in Omega Cen</title><shortName>J/AJ/152/170</shortName><identifier>ivo://CDS.VizieR/J/AJ/152/170</identifier><altIdentifier>doi:10.26093/cds/vizier.51520170</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Braga V.F.</name></creator><creator><name>Stetson P.B.</name></creator><creator><name>Bono G.</name></creator><creator><name>Dall'Ora M.</name></creator><creator><name>Ferraro I.</name></creator><creator><name>Fiorentino G.,Freyhammer L.M.</name></creator><creator><name>Iannicola G.</name></creator><creator><name>Marengo M.</name></creator><creator><name>Neeley J.</name></creator><creator><name>Valenti E.,Buonanno R.</name></creator><creator><name>Calamida A.</name></creator><creator><name>Castellani M.</name></creator><creator><name>da Silva R.</name></creator><creator><name>Degl'Innocenti S.,Di Cecco A.</name></creator><creator><name>Fabrizio M.</name></creator><creator><name>Freedman W.L.</name></creator><creator><name>Giuffrida G.</name></creator><creator><name>Lub J.</name></creator><creator><name>Madore B.F.,Marconi M.</name></creator><creator><name>Marinoni S.</name></creator><creator><name>Matsunaga N.</name></creator><creator><name>Monelli M.</name></creator><creator><name>Persson S.E.,Piersimoni A.M.</name></creator><creator><name>Pietrinferni A.</name></creator><creator><name>Prada-Moroni P.</name></creator><creator><name>Pulone L.,Stellingwerf R.</name></creator><creator><name>Tognelli E.</name></creator><creator><name>Walker A.R.</name></creator><date role="Updated">2019-12-27T04:38:40Z</date><date role="Created">2018-03-28T10:38:21Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>metallicity</subject><description>New accurate and homogeneous optical UBVRI photometry has been obtained for variable stars in the Galactic globular cluster {omega} Cen (NGC 5139). We secured 8202 CCD images covering a time interval of 24 years and a sky area of 84x48arcmin. The current data were complemented with data available in the literature and provided new, homogeneous pulsation parameters (mean magnitudes, luminosity amplitudes, periods) for 187 candidate {omega} Cen RR Lyrae (RRLs). Among them we have 101 RRc (first overtone) and 85 RRab (fundamental) variables, and a single candidate RRd (double-mode) variable. Candidate Blazhko RRLs show periods and colors that are intermediate between the RRc and RRab variables, suggesting that they are transitional objects. A comparison of the period distribution and the Bailey diagram indicates that RRLs in {omega} Cen show a long-period tail not present in typical Oosterhoff II (OoII) globulars. The RRLs in dwarf spheroidals and in ultra-faint dwarfs have properties between Oosterhoff intermediate and OoII clusters. Metallicity plays a key role in shaping the above evidence. These findings do not support the hypothesis that {omega} Cen is the core remnant of a spoiled dwarf galaxy. Using optical period-Wesenheit relations that are reddening-free and minimally dependent on metallicity we find a mean distance to {omega} Cen of 13.71+/-0.08+/-0.01mag (semi-empirical and theoretical calibrations). Finally, we invert the I-band period-luminosity-metallicity relation to estimate individual RRLs' metal abundances. The metallicity distribution agrees quite well with spectroscopic and photometric metallicity estimates available in the literature.</description><source format="bibcode">2016AJ....152..170B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/152/170</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/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/576/A30">J/A+A/576/A30 : Light-curve templates for classical Cepheids (Inno+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/583/A76">J/A+A/583/A76 : Om. 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ivo-id="ivo://CDS.VizieR/J/A+A/505/117">J/A+A/505/117 : Abundances of red giants in 15 globulars (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/959">J/A+A/493/959 : UBV(RI)cHalpha photometry in omega Cen (Bellini+, 2009)</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/ApJ/698/2048">J/ApJ/698/2048 : Abundances of red giants in {omega} Cen (Johnson+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/506">J/AJ/136/506 : Radial velocities of {omega} Cen members (Da Costa+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1447">J/AJ/133/1447 : Light curves of variables in {omega} Cen (Weldrake+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/1021">J/ApJ/663/1021 : Log of {omega} Cen scientific images (Castellani+, 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Pulsation period based on a compilation of literature values (Clement et al. 2001AJ....122.2587C) (3)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Per2</name><description>[0.25/1.1]? Pulsation period based on the current estimate using the Lomb-Scargle (LS) method (Scargle 1982ApJ...263..835S)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Band1</name><description>[BVRI] Band used for the epoch of light maximum (T_0_(max)) (B, V, R, or I)</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HJD1</name><description>[49113.5/54273.5]? 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Photometric quality index of the R-band light curve (q_R_) (4)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>qI</name><description>[0/3]? Photometric quality index of the I-band light curve (q_I_) (4)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Mode</name><description>Pulsation mode identification (RRab, RRc, or RRd) (5)</description><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>f_Mode</name><description>[*] An asterisk flag on Mode indicates that the variable is candidate Blazhko RR Lyrae</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/AJ/152/170/table10</name><description>Metallicity estimates ([Fe/H]) of candidate {omega} Cen RR Lyrae (RRLs) based on spectroscopy (Sollima et al. 2006, Cat. J/ApJ/640/L43) and on photometric indices (Rey et al. 2000, Cat. J/AJ/119/1824, ours)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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J/AJ/119/1824) and on the current estimates (4)</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S06+Rey+PLI</name><description>[0/0.8] Error in S06+Rey+PLI</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/152/170/notes</name><description>Notes</description><column><name>Note</name><description>Notes about the star</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="393*">char</dataType></column><column><name>Name</name><description>Name of the {omega} Cen RR Lyrae</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">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></table></schema></tableset></ri:Resource>