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<ri:Resource created="2003-08-22T13:25:24Z" 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>C stars in Pegasus, DDO 210 and Tucana</title><shortName>J/AJ/120/1801</shortName><identifier>ivo://CDS.VizieR/J/AJ/120/1801</identifier><altIdentifier>doi:10.26093/cds/vizier.51201801</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Battinelli P.</name></creator><creator><name>Demers S.</name></creator><date role="Updated">2023-04-06T16:50:39Z</date><date role="Created">2003-08-22T13:25:24Z</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>carbon-stars</subject><subject>visible-astronomy</subject><subject>kron-cousins-photometry</subject><subject>ccd-photometry</subject><description>We present the latest results of our ongoing four-filter photometric survey of C stars in Local Group dwarf irregular galaxies. Observations of the two low-luminosity dwarf irregular galaxies, Pegasus and DDO 210, revealed 40 and three C stars, respectively, assuming that the reddening of Pegasus is negligible. No C stars were identified in Tucana. Our observations permit the estimation of the color-magnitude diagram contamination by foreground M dwarfs thus yielding reliable C/M ratios. Our R and I photometry of the C stars cannot be used to solve the extinction controversy toward Pegasus. The three C stars in DDO 210 are quite bright when compared with C star populations in other dwarf galaxies. A larger, fainter population in that galaxy seems improbable, however. The statistics of C stars currently on hand for dwarf galaxies show a well-defined trend with the absolute magnitude of dwarf galaxies.</description><source format="bibcode">2000AJ....120.1801B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/120/1801</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/119/2780">J/AJ/119/2780 : C stars in IC 1613 (Albert+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/832">J/AJ/123/832 : C star population in NGC 6822 (Letarte+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/1298">J/AJ/125/1298 : C star population in outer disk of M31 (Battinelli+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/410/795">J/A+A/410/795 : Photometry of NGC 3109 carbon stars (Demers+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/3037">J/AJ/125/3037 : RI photometry of NGC 205 carbon stars (Demers+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/111">J/A+A/416/111 : C stars in Wolf-Lundmark-Melotte galaxy (Battinelli+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/417/479">J/A+A/417/479 : RI photometry of NGC 185 carbon stars (Battinelli+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/418/33">J/A+A/418/33 : RI photometry of C stars in NGC 147 (Battinelli+, 2004)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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