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<ri:Resource created="2012-04-02T12:54:27Z" 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>Spectropolarimetry of 60 Cyg and {pi} Aqr</title><shortName>J/ApJ/709/1306</shortName><identifier>ivo://CDS.VizieR/J/ApJ/709/1306</identifier><altIdentifier>doi:10.26093/cds/vizier.17091306</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wisniewski J.P.</name></creator><creator><name>Draper Z.H.</name></creator><creator><name>Bjorkman K.S.</name></creator><creator><name>Meade M.R.</name></creator><creator><name>Bjorkman J.E.,Kowalski A.F.</name></creator><date role="Updated">2017-07-05T07:00:06Z</date><date role="Created">2012-04-02T12:54:27Z</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>line-intensities</subject><subject>polarimetry</subject><description>Classical Be stars are known to occasionally transition from having a gaseous circumstellar disk ("Be phase") to a state in which all observational evidence for the presence of these disks disappears ("normal B-star phase"). We present one of the most comprehensive spectropolarimetric views to date of such a transition for two Be stars, {pi} Aquarii and 60 Cygni. The disk-loss episode of 60 Cyg was characterized by a generally monotonic decrease in emission strength over a timescale of ~1000 days from the maximum V-band polarization to the minimum H{alpha} equivalent width, consistent with the viscous timescale of the disk, assuming {alpha}~0.14. {pi} Aqr's disk loss was episodic in nature and occurred over a timescale of ~2440 days.</description><source format="bibcode">2010ApJ...709.1306W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/709/1306</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/II/226">II/226 : Stellar polarization catalogs agglomeration (Heiles, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/220">II/220 : Polarisation of Be stars (McDavid, 1986-1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/187/228">J/ApJS/187/228 : H{alpha} profiles of Be stars (Silaj+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/912">J/A+A/368/912 : Polarization and rotational velocities of Be stars (Yudin,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/378/861">J/A+A/378/861 : Spectroscopy of Be stars (Chauville+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/106/949">J/PASP/106/949 : Multicolor polarimetry of Be stars (McDavid, 1994)</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/ApJ/709/1306</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/709/1306</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/709/1306</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/709/1306</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/709/1306</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/709/1306</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/ApJ/709/1306/table1</name><description>Summary of 60 Cyg data</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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