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<ri:Resource created="2006-09-13T18:42:02Z" 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>Effective temperature of B stars</title><shortName>J/A+A/444/941</shortName><identifier>ivo://CDS.VizieR/J/A+A/444/941</identifier><altIdentifier>doi:10.26093/cds/vizier.34440941</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Paunzen E.</name></creator><creator><name>Schnell A.</name></creator><creator><name>Maitzen H.M.</name></creator><date role="Updated">2017-10-12T12:59:41Z</date><date role="Created">2006-09-13T18:42:02Z</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>b-stars</subject><subject>effective-temperature</subject><subject>photometry</subject><description>We establish an empirical effective temperature calibration of main sequence, luminosity class V to III B-type stars for the Delta a photometric system which was originally developed to detect magnetic chemically peculiar objects of the upper main sequence (early B-type to early F-type) at 5200A. However, this system provides the index g1-y which shows an excellent correlation with B-V as well as b-y and can be used as an indicator of the effective temperature. This is supplemented by a very accurate color-magnitude diagram, y or V versus g1-y, which can be used, for example, to determine the reddening, distance and age of an open cluster. This makes the Delta a photometric system an excellent tool to investigate the HR diagram in more detail. Using the reddening-free parameters and already established calibrations within the Stromgren uvbybeta, Geneva 7-color and Johnson UBV systems, a polynomial fit of third degree for the averaged effective temperatures to the individual (g1-y)0 values was derived. For this purpose, data from the literature as well as new observations were taken resulting in 225 suitable bright normal B-type objects. The statistical mean of the error for this sample is 238K which is sufficient to investigate the HRD of distant galactic open clusters as well as extragalactic aggregates in the future.</description><source format="bibcode">2005A&amp;A...444..941P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/444/941</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/A+A/391/1039">J/A+A/391/1039 : Teff of metal-poor A-type stars (Kinman+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/411/559">J/A+A/411/559 : Teff for 181 F-K dwarfs (Kovtyukh+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/429/235">J/A+A/429/235 : Teff of 119 C-rich giants (Bergeat+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/442/281">J/A+A/442/281 : Late-type giants BVRIJHKL and Teff calibration</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/117/227">J/A+AS/117/227 : Dwarf effective temperatures (Alonso+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/122/131">J/A+AS/122/131 : Delta Scuti rotational velocities and Teff (Solano+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/626/446">J/ApJ/626/446 : Teff scale of FGK stars (Ramirez+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/BSAO/38.152">J/other/BSAO/38.152 : Teff of CP stars (Glagolevskij 1994)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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