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<ri:Resource created="2023-01-16T15:39:29Z" status="active" updated="2025-06-13T15:25:00Z" 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>1997-2019 automated B,V phot. of gam Cas</title><shortName>J/ApJ/915/13</shortName><identifier>ivo://CDS.VizieR/J/ApJ/915/13</identifier><altIdentifier>doi:10.26093/cds/vizier.19150013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Smith M.A.</name></creator><creator><name>Henry G.W.</name></creator><date role="Updated">2023-03-20T14:23:30Z</date><date role="Created">2023-01-16T15:39:29Z</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>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>be-stars</subject><description>{gamma} Cassiopeiae (B0.5IVe) is the noted prototype of a subgroup of classical Be stars exhibiting hard thermal X-ray emission. This paper reports results from a 23yr optical campaign on this star with an automated photometric telescope (APT). A series of unstable long cycles of length 56-91days has nearly ceased over the last decade. Also, we revise the frequency of the dominant coherent signal at 0.82238/days. This signal's amplitude has nearly disappeared in the last 15yr but has somewhat recovered its former strength. We confirm the presence of secondary nonradial pulsation signals found by other authors at frequencies 1.24, 2.48, and 5.03days^-1^. The APT data from intensively monitored nights reveal rapidly variable amplitudes among these frequencies. We show that peculiarities in the 0.82days^-1^ waveform exist that can vary even over several days. Although the 0.82days^-1^ frequency is near the star's presumed rotational frequency, because of its phase slippage with respect to a dip pattern in its far-UV light curve, it is preferable to consider the UV pattern, not the 0.82days^-1^ signal, as associated with rotational modulation. We also find hints of the UV dip pattern in periodograms of seasonal data early in our program.</description><source format="bibcode">2021ApJ...915...13S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/915/13</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/647/1375">J/ApJ/647/1375 : BV light curves of {gamma} Cas (Smith+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/1280">J/ApJ/686/1280 : Discovery of hot subdwarf companion to FY CMa (Peters+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/760/10">J/ApJ/760/10 : BV light curves of {gamma} Cas (1997-2011) (Henry+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A59">J/A+A/537/A59 : Radial velocities of gamma Cas (Nemravov+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A53">J/A+A/540/A53 : {gamma} Cas radial velocity curve (Smith+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/2">J/ApJ/765/2 : FUV radial velocities of 59 Cyg (Peters+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/613/A70">J/A+A/613/A70 : Be stars in the exofield of CoRoT. II. (Semaan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/640/A36">J/A+A/640/A36 : OB stars TESS phot. &amp; high-res. spectroscopy (Bowman+, 2020)</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/915/13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/915/13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/915/13</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/915/13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/915/13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/915/13</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/915/13/table1</name><description>Photometric observations of {gamma} Cas for seasons 1997-2019</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>HJD</name><description>[50718.69/58888.6] Reduced Julian Date; HJD-2400000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>VarB</name><description>[-4.4/-4.2]? Variable - Comparison (HD 6210) differential magnitude in B (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VarV</name><description>[-3.8/-3.6]? Variable - Comparison (HD 6210) differential magnitude in V (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ChkB</name><description>[-0.83/-0.78]? Check (HD 5395) - Comparison differential magnitude in B (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ChkV</name><description>[-1.25/-1.19]? Check (HD 5395) - Comparison differential magnitude in V (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>