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<ri:Resource created="2012-03-15T06:55:49Z" 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>Walraven photometry in Sco-Cen association</title><shortName>J/A+A/216/44</shortName><identifier>ivo://CDS.VizieR/J/A+A/216/44</identifier><altIdentifier>doi:10.26093/cds/vizier.32160044</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>De Geus E.J.</name></creator><creator><name>De Zeeuw P.T.</name></creator><creator><name>Lub J.</name></creator><date role="Updated">2019-07-29T14:15:13Z</date><date role="Created">2012-03-15T06:55:49Z</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>stellar-associations</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>effective-temperature</subject><description>Walraven photometry is presented of established and probable members of the Scorpio-Centaurus OB association. For each star, effective temperature and surface gravity are derived using Kurucz atmosphere models (1979ApJS...40....1K). From the Straizys and Kuriliene (1981Ap&amp;SS..80..353S) tables, absolute magnitudes are calculated. Distance moduli and visual extinctions are determined for all stars. From a comparison of the HR-diagrams of the stars in each subgroup with theoretical isochrones, the ages of the three subgroups are derived. The distances to the three subgroups are shown to be different; there is a general trend (also within each subgroup) for the distances to be larger at higher galactic longitudes. The visual extinction in the youngest subgroup Upper-Scorpius, is well correlated with the IRAS 100-micron map. The distance toward the Ophiuchus dark clouds is found to be 125 pc, based on the photometric distances to the stars. Most of the early-type stars in Upper-Scorpius are located at the far side of the dark clouds.</description><source format="bibcode">1989A&amp;A...216...44D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/216/44</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/ApJS/82/117">J/ApJS/82/117 : UBV and H-{beta} in Sco-Cen association (Slawson+, 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/356/541">J/A+A/356/541 : T Tauri stars in the Sco-Cen OB association (Koehler+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/448/1001">J/A+A/448/1001 : Radial velocities of B stars in Sco-Cen (Jilinski+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/1670">J/AJ/124/1670 : Post-T Tauri Stars in Sco-Cen Association (Mamajek+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/33/643">J/PAZh/33/643 : Kinematics of Sco-Cen OB Association (Bobylev+, 2007)</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/A+A/216/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/216/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/216/44</mirrorURL></interface></capability><capability><interface 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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>HD</name><description>HD number of the star</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Glon</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>Glat</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[B-U]</name><description>Reddenning-free parameter (B-U)-0.61(V-B) (1)</description><unit>mag</unit><ucd>phot.color.reddFree</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[U-W]</name><description>Reddenning-free parameter (U-W)-0.45(V-B) (1)</description><unit>mag</unit><ucd>phot.color.reddFree</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[B-L]</name><description>Reddenning-free parameter (B-L)-0.39(V-B) (1)</description><unit>mag</unit><ucd>phot.color.reddFree</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logTe</name><description>Effective temperature (from photometry)</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logg</name><description>Gravity (from photometry)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL</name><description>Luminosity (in solar units)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>mv</name><description>Johnson V magnitude (estimated {sigma}=0.015)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mv</name><description>Absolute magnitude</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Av</name><description>Absorption (assuming R=3.2)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DM</name><description>Distance modulus DM = mv-MV+Av+5 (estimated {sigma}=0.3)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Heliocentric distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Mmb</name><description>[Mm] Membership: M=member from proper motion, m=member from photometry, blank=non-member (2)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SpType</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>