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<ri:Resource created="2006-08-11T14:12:00Z" status="active" updated="2025-09-29T20:17:23Z" 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>Extinction of OB stars</title><shortName>J/AN/324/219</shortName><identifier>ivo://CDS.VizieR/J/AN/324/219</identifier><altIdentifier>doi:10.26093/cds/vizier.113240219</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wegner W.</name></creator><date role="Updated">2025-09-29T20:17:23Z</date><date role="Created">2006-08-11T14:12:00Z</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>early-type-stars</subject><subject>photometry</subject><subject>extinction</subject><description>The paper presents an extensive list of the total to selective extinction ratios R calculated from the infrared magnitudes of 597 O and B stars using the extrapolation method. The IR magnitudes of these stars were taken from the literature. The IR colour excesses are determined with the aid of "artificial standards", Wegner (1994MNRAS.270..229W). The individual and mean values of total to selective extinction ratios R differ in most cases from the average value R=3.10+/-0.05, Wegner (1993AcA....43..209W) in different OB associations. The relation between total to selective extinction ratios R determined in this paper and those calculated using the "method of variable extinction" and the Cardelli et al. (1989ApJ...345..245C) formulae is discussed. The R values presented in this paper can be used to determine individual absolute magnitudes of reddened OB stars with known trigonometric parallaxes.</description><source format="bibcode">2003AN....324..219W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AN/324/219</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/62">II/62 : Catalogue of Extinction Data (Neckel+, 1980)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/BaltA/11/1">J/BaltA/11/1 : Interstellar extinction curves of OB stars (Wegner 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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>Name</name><description>Star name (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Vmag</name><description>V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpType</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>r_SpType</name><description>References for SpType, in refs.dat file</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>E(B-V)</name><description>Extinction in B-V</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_E(B-V)</name><description>References for UBV data, in refs.dat file</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R</name><description>Total-to-selective extinction ratio, R=A(V)/E(B-V)</description><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R</name><description>rms uncertainty on R</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VMAG</name><description>? 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