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<ri:Resource created="2016-08-24T12:23:49Z" 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>The pulsations of G 207-9 and LP 133-144</title><shortName>J/MNRAS/461/4059</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/461/4059</identifier><altIdentifier>doi:10.26093/cds/vizier.74614059</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bognar Zs.</name></creator><creator><name>Paparo M.</name></creator><creator><name>Molnar L.</name></creator><creator><name>P. I. Papics</name></creator><creator><name>Plachy E.</name></creator><creator><name>Verebelyi E.,Sodor A.</name></creator><date role="Updated">2024-08-16T20:17:59Z</date><date role="Created">2016-08-24T12:23:49Z</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>variable-stars</subject><subject>white-dwarf-stars</subject><subject>ccd-photometry</subject><description>G 207-9 and LP 133-144 are two rarely observed ZZ Ceti stars located in the middle and close to the blue edge of the ZZ Ceti instability domain, respectively. We aimed to observe them at least during one observing season at Konkoly Observatory with the purpose of extending the list of known pulsation modes for asteroseismic investigations and detect any significant changes in their pulsational behaviour. We determined five and three new normal modes of G 207-9 and LP 133-144, respectively. In LP 133-144, our frequency analysis also revealed that at least at three modes there are actually triplets with frequency separations of ~4Hz. The rotational period of LP 133-144 based on the triplets is ~=42h. The preliminary asteroseismic fits of G 207-9 predict Teff=12000 or 12400K and M=0.855--0.870M_{sun}_ values for the effective temperature and mass of the star, depending on the assumptions on the spherical degree (l) values of the modes. These results are in agreement with the spectroscopic determinations. In the case of LP 133-144, the best-fitting models prefer Teff=11800K in effective temperature and M*&gt;=0.71M_{sun}_ stellar masses, which are more than 0.1M_{sun}_ larger than the spectroscopic value.</description><source format="bibcode">2016MNRAS.461.4059B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/461/4059</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/631/1100">J/ApJ/631/1100 : Atmospheric parameters of DA white dwarfs (Gianninas+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/528/A147">J/A+A/528/A147 : CoRoT 101155310 light curve (Poretti+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/570/A116">J/A+A/570/A116 : Monitoring of the V777 Her star KUV 05134+2605 (Bognar+, 2014)</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/MNRAS/461/4059</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/461/4059</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/461/4059</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/461/4059</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/461/4059</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/461/4059</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"/></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/461/4059/g207</name><description>CCD observations of G 207-9 at Konkoly observatory</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>BJD</name><description>Barycentric Julian dates in Barycentric Dynamical Time (BJD_TDB)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dmag</name><description>Differential magnitude</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/MNRAS/461/4059/lp133</name><description>CCD observations of LP 133-144 at Konkoly observatory</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>BJD</name><description>Barycentric Julian dates in Barycentric Dynamical Time (BJD_TDB)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dmag</name><description>Differential magnitude</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>