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<ri:Resource created="2015-07-28T14:33:11Z" 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>{Delta}a observations of 3 globular clusters</title><shortName>J/MNRAS/443/2492</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/443/2492</identifier><altIdentifier>doi:10.26093/cds/vizier.74432492</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Paunzen E.</name></creator><creator><name>Iliev I.KH.</name></creator><creator><name>Pintado O.I.</name></creator><creator><name>Baum H.</name></creator><creator><name>Maitzen H.M.</name></creator><creator><name>Netopil M.,Onehag A.</name></creator><creator><name>Zejda M.</name></creator><creator><name>Fraga L.</name></creator><date role="Updated">2024-08-10T20:18:12Z</date><date role="Created">2015-07-28T14:33:11Z</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>photometry</subject><description>Globular clusters are main astrophysical laboratories to test and modify evolutionary models. Thought to be rather homogeneous in their local elemental distribution of members, results suggest a wide variety of chemical peculiarities. Besides different main sequences, believed to be caused by different helium abundances, peculiarities of blue horizontal-branch stars and on the red giant branch were found. This whole zoo of peculiar objects has to be explained in the context of stellar formation and evolution. The tool of {Delta}a photometry is employed in order to detect peculiar stars in the whole spectral range. This three filter narrow-band system measures the flux distribution in the region from 4900 to 5600{AA} in order to find any peculiarities around 5200{AA}. It is highly efficient to detect classical chemically peculiar stars of the upper main sequence, Be/Ae, shell and metal-weak objects in the Milky Way and Magellanic Clouds. We present {Delta}a photometry of 2266 stars from 109 individual frames for three globular clusters (NGC 104, NGC 6205, and NGC 7099). A comparison with published abundances, for three horizontal-branch stars, only, yields an excellent agreement. According to the 3{sigma} detection limit of each globular cluster, about 3 percent of the stars lie in abnormal regions in the diagnostic diagrams. The first observations of three widely different aggregates give very promising results, which will serve as a solid basis for follow-up observations including photometric as well as spectroscopic studies.</description><source format="bibcode">2014MNRAS.443.2492P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/443/2492</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/248">II/248 : UBV photometry and proper motions in M13 (Kadla, 1966)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/1061">J/AJ/112/1061 : BV photometry of NGC 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2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/50">J/AJ/143/50 : White dwarfs in 47 Tuc (NGC 104) with HST (Woodley+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/L38">J/ApJ/754/L38 : Abundances and radial velocities of M13 giants (Johnson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A36">J/A+A/555/A36 : VrI light curves of NGC7099 variables (Kains+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/148">J/ApJ/772/148 : Blue straggler and red giant stars in M30 (Lovisi+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/A58">J/A+A/566/A58 : Radial velocities in M3, M13, and M92 (Kamann+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/780/94">J/ApJ/780/94 : Abundances of red giants in 47 Tuc (Cordero+, 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