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<ri:Resource created="2015-04-14T12:25:14Z" 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>VVV globulars. I. 2MASS-GC 02, Terzan 10</title><shortName>J/AJ/149/99</shortName><identifier>ivo://CDS.VizieR/J/AJ/149/99</identifier><altIdentifier>doi:10.26093/cds/vizier.51490099</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Alonso-Garcia J.</name></creator><creator><name>Dekany I.</name></creator><creator><name>Catelan M.</name></creator><creator><name>Ramos R.C.</name></creator><creator><name>Gran F.</name></creator><creator><name>Amigo P.,Leyton P.</name></creator><creator><name>Minniti D.</name></creator><date role="Updated">2017-11-06T12:23:56Z</date><date role="Created">2015-04-14T12:25:14Z</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>stellar-distance</subject><subject>infrared-photometry</subject><description>The VISTA Variables in the Via Lactea (VVV) ESO Public Survey is opening a new window to study inner Galactic globular clusters (GCs) using their variable stars. These GCs have been neglected in the past due to the difficulties caused by the presence of elevated extinction and high field stellar densities in their lines of sight. However, the discovery and study of any present variables in these clusters, especially RR Lyrae stars, can help to greatly improve the accuracy of their physical parameters. It can also help to shed some light on the questions raised by the intriguing Oosterhoff dichotomy in the Galactic GC system. In a series of papers we plan to explore variable stars in the GCs falling inside the field of the VVV survey. In this first paper, we search for and study the variables present in two highly reddened, moderately metal-poor, faint, inner Galactic GCs: 2MASS-GC 02 and Terzan 10. We report the discovery of sizable populations of RR Lyrae stars in both GCs. We use near-infrared period-luminosity relations to determine the color excess of each RR Lyrae star, from which we obtain both accurate distances to the GCs and the ratios of the selective-to-total extinction in their directions. We find the extinction toward both clusters to be elevated, non-standard, and highly differential. We also find both clusters to be closer to the Galactic center than previously thought, with Terzan 10 being on the far side of the Galactic bulge. Finally, we discuss their Oosterhoff properties, and conclude that both clusters stand out from the dichotomy followed by most Galactic GCs.</description><source format="bibcode">2015AJ....149...99A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/149/99</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/II/337">II/337 : VISTA Variables in the Via Lactea Survey DR1 (Minniti+, 2014)</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/A+A/571/A36">J/A+A/571/A36 : M dwarfs in b201 tile of VVV survey (Rojas-Ayala+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/L9">J/A+A/564/L9 : Near-IR photometry in VVV CL08 (Ramirez Alegria+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A115">J/A+A/562/A115 : VVV: star formation and embedded clusters (Solin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/554/A123">J/A+A/554/A123 : Near-IR catalog of novae in VVV survey area (Saito+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/429/385">J/MNRAS/429/385 : Short-period variables near Galactic Centre</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/552/A74">J/A+A/552/A74 : NIR photometry of Galactic PNe with VVV Survey</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/127">J/AJ/144/127 : 204 galaxy candidates from VVV infrared photometry</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/70">J/AJ/143/70 : Differential reddening in MW globulars (Alonso-Garcia+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/532/A131">J/A+A/532/A131 : New Galactic star clusters in VVV survey (Borissova+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/474/121">J/A+A/474/121 : Galactic globular cluster 2MASS GC02 JKs photometry</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/126/319">J/A+AS/126/319 : Terzan 10, ESO456-SC38, UKS 1 VIz photometry (Ortolani+ 1997)</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/AJ/149/99</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/149/99</mirrorURL><mirrorURL 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