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<ri:Resource created="2014-05-28T08:04:14Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Differential BV photometry of {delta} Sco</title><shortName>J/AJ/145/142</shortName><identifier>ivo://CDS.VizieR/J/AJ/145/142</identifier><altIdentifier>doi:10.26093/cds/vizier.51450142</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jones C.E.</name></creator><creator><name>Wiegert P.A.</name></creator><creator><name>Tycner C.</name></creator><creator><name>Henry G.W.</name></creator><creator><name>Cyr R.P.</name></creator><creator><name>Halonen R.J.,Muterspaugh M.W.</name></creator><date role="Updated">2017-06-20T13:17:21Z</date><date role="Created">2014-05-28T08:04:14Z</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>be-stars</subject><subject>multiple-stars</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We acquired Johnson BV photometry of the binary Be disk system {delta} Scorpii during its 2009, 2010, 2011, and 2012 observing seasons and used it to probe the innermost regions of the disk. We found that several disk building events have occurred during this time, resulting in an overall brightening in the V band and reddening of the system. In addition to these long-term trends, we found cyclical variability in each observing season on timescales between 60 and 100days. We were able to reproduce the changes in the magnitude and color of {delta} Sco using our theoretical models and found that variable mass-loss rates in the range 2.5-7.0*10^-9^M_{Sun}_/yr over ~35days can reproduce the observed increase in brightness.</description><source format="bibcode">2013AJ....145..142J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/145/142</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/729/L5">J/ApJ/729/L5 : The revised orbit of the {delta} Sco system (Tycner+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1727">J/AJ/127/1727 : Differential magnitudes of binary stars (Horch+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/408/305">J/A+A/408/305 : Spectroscopic observations of delta Sco (Miroshnichenko+, 2003)</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/AJ/145/142</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/145/142</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/145/142</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/145/142</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/145/142</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/145/142</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/145/142/table1</name><description>Photometric observations of {delta} Sco (2009-2012)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RJD</name><description>[54857/56102] Reduced Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DBmag</name><description>[-2.199/-1.811]? Variable-Comparison differential B-band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DVmag</name><description>[-2.253/-1.753]? Variable-Comparison differential V-band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.V;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DBmag2</name><description>[-1.497/-1.445]? Check-Comparison differential B-band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DVmag2</name><description>[-1.466/-1.41]? Check-Comparison differential V-band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.V;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>