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<ri:Resource created="2017-07-13T15:30:57Z" 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>Spectropolarimetric survey of classical Be stars</title><shortName>J/ApJ/786/120</shortName><identifier>ivo://CDS.VizieR/J/ApJ/786/120</identifier><altIdentifier>doi:10.26093/cds/vizier.17860120</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Draper Z.H.</name></creator><creator><name>Wisniewski J.P.</name></creator><creator><name>Bjorkman K.S.</name></creator><creator><name>Meade M.R.</name></creator><creator><name>Haubois X.,Mota B.C.</name></creator><creator><name>Carciofi A.C.</name></creator><creator><name>Bjorkman J.E.</name></creator><date role="Updated">2017-08-22T08:35:42Z</date><date role="Created">2017-07-13T15:30:57Z</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>stellar-spectral-types</subject><subject>effective-temperature</subject><subject>polarimetry</subject><subject>line-intensities</subject><description>Recent observational and theoretical studies of classical Be stars have established the utility of polarization color diagrams (PCDs) in helping to constrain the time-dependent mass decretion rates of these systems. We expand on our pilot observational study of this phenomenon, and report the detailed analysis of a long-term (1989-2004) spectropolarimetric survey of nine additional classical Be stars, including systems exhibiting evidence of partial disk-loss/disk-growth episodes as well as systems exhibiting long-term stable disks. After carefully characterizing and removing the interstellar polarization along the line of sight to each of these targets, we analyze their intrinsic polarization behavior. We find that many steady-state Be disks pause at the top of the PCD, as predicted by theory. We also observe sharp declines in the Balmer jump polarization for later spectral type, near edge-on steady-state disks, again as recently predicted by theory, likely caused when the base density of the disk is very high, and the outer region of the edge-on disk starts to self absorb a significant number of Balmer jump photons. The intrinsic V-band polarization and polarization position angle of {gamma} Cas exhibits variations that seem to phase with the orbital period of a known one-armed density structure in this disk, similar to the theoretical predictions of Halonen &amp; Jones. We also observe stochastic jumps in the intrinsic polarization across the Balmer jump of several known Be+sdO systems, and speculate that the thermal inflation of part of the outer region of these disks could be responsible for producing this observational phenomenon. Finally, we estimate the base densities of this sample of stars to be between ~8x10^-11^ and ~4x10^-12^ g/cm^3^ during quasi steady state periods given there maximum observed polarization.</description><source format="bibcode">2014ApJ...786..120D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/786/120</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/220">II/220 : Polarisation of Be stars (McDavid, 1986-1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/106/949">J/PASP/106/949 : Multicolor polarimetry of Be stars (McDavid, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/912">J/A+A/368/912 : Polarization and rotational velocities of Be stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/440/305">J/A+A/440/305 : Fundamental parameters of fast-rotating B stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/459/137">J/A+A/459/137 : Bright Be shell stars (Rivnius+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/1306">J/ApJ/709/1306 : Spectropolarimetry of 60 Cyg and {pi} Aqr</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/BASI/39.517">J/other/BASI/39.517 : Spectroscopy of classical Be stars (Mathew+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A79">J/A+A/550/A79 : H{alpha} and H{beta} lines of northern Be stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/768/128">J/ApJ/768/128 : K-band calibrated visibilities of 24 Be stars</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/786/120</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/786/120</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/786/120</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/786/120</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/786/120</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/786/120</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/786/120/table1 (Target Star Summary)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/786/120/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/786/120/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/786/120/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>239.5473694</ra><dec>-14.2793581</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1769 2884 3030 14631 15372 15375 19202 22911 31759 39922 44502</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/786/120?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/786/120/table2</name><description>Raw HPOL Data</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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