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<ri:Resource created="2012-07-03T14:48:57Z" 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>Early asteroseismic results from Kepler</title><shortName>J/ApJ/718/L97</shortName><identifier>ivo://CDS.VizieR/J/ApJ/718/L97</identifier><altIdentifier>doi:10.26093/cds/vizier.17189097</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Van Grootel V.</name></creator><creator><name>Charpinet S.</name></creator><creator><name>Fontaine G.</name></creator><creator><name>Brassard P.</name></creator><creator><name>Green E.M.,Randall S.K.</name></creator><creator><name>Silvotti R.</name></creator><creator><name>Ostensen R.H.</name></creator><creator><name>Kjeldsen H.,Christensen-Dalsgaard J.</name></creator><creator><name>Borucki W.J.</name></creator><creator><name>Koch D.</name></creator><date role="Updated">2018-01-30T07:17:50Z</date><date role="Created">2012-07-03T14:48:57Z</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>b-stars</subject><subject>variable-stars</subject><description>We present a seismic analysis of the pulsating hot B subdwarf KPD 1943+4058 (KIC 005807616) on the basis of the long-period, gravity-mode pulsations recently uncovered by Kepler. This is the first time that g-mode seismology can be exploited quantitatively for stars on the extreme horizontal branch, all previous successful seismic analyses having been confined so far to short-period, p-mode pulsators. We demonstrate that current models of hot B subdwarfs can quite well explain the observed g-mode periods, while being consistent with independent constraints provided by spectroscopy. We identify the 18 pulsations retained in our analysis as low-degree ({l}=1 and 2), intermediate-order (k=-9 through -58) g-modes. The periods (frequencies) are recovered, on average, at the 0.22% level, which is comparable to the best results obtained for p-mode pulsators. We infer the following structural and core parameters for KPD 1943+4058 (formal fitting uncertainties only): T_eff_=28050+/-470K, logg=5.52+/-0.03, M_*_=0.496+/-0.002M_{sun}_, log(M_env_/M*)=-2.55+/-0.07, log(1-M_core_/M_*_)=-0.3+/-0.01, and X_core_(C+O)=0.261+/-0.008. We additionally derive the age of the star since the zero-age extended horizontal branch 18.4+/-1.0Myr, the radius R=0.203+/-0.007R_{sun}_, the luminosity L=22.9+/-3.13L_{sun}_, the absolute magnitude M_V_=4.21+/-0.11, the reddening index E(B-V)=0.094+/-0.017, and the distance d=1180+/-95pc.</description><source format="bibcode">2010ApJ...718L..97V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/718/L97</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/A+A/525/A23">J/A+A/525/A23 : Frequency analysis of HD 49434 (Mathias+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/471">J/A+A/506/471 : Frequency analysis of CoRoT B stars (Degroote+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/111">J/A+A/506/111 : Frequency analysis of HD 180642 (V1449 Aql) (Degroote+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/79">J/A+A/506/79 : Asteroseismic analysis of HD 174936 (Garcia Hernandez+, 2009)</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/718/L97</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/718/L97</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/718/L97</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/718/L97</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/718/L97</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/718/L97</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/718/L97/table2</name><description>Mode identification and other properties</description><column><name>k</name><description>[-63/-3] Radial order</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>l</name><description>[1/4] Degree</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nuObs</name><description>? Observed frequency</description><unit>uHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>nuTh</name><description>Theoretical frequency</description><unit>uHz</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PObs</name><description>? 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Period dispersion {Delta}P</description><unit>s</unit><ucd>time.period;instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Delnu</name><description>? Frequency dispersion {Delta}{nu}</description><unit>uHz</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ID</name><description>Mode identification (f_1_-f_27_, u_1_-u_14_)</description><ucd>meta.id;stat.fit</ucd></column><column><name>f_ID</name><description>[1/2] Flag on ID (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/ApJ/718/L97/table1</name><description>List of frequencies f_n_ (n is by order of decreasing amplitude) detected in KPD 1943+4058</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>ID</name><description>Mode identification (f_1_-f_27_, u_1_-u_14_)</description><ucd>meta.id;stat.fit</ucd><flag>primary</flag></column><column><name>f_ID</name><description>[*] *: pulsation period safely assumed to be independent (18 periods used in the analysis)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Per</name><description>Period</description><unit>s</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Freq</name><description>Frequency</description><unit>uHz</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S/N</name><description>Signal to noise ratio</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Comm</name><description>Comments</description><ucd>meta.note</ucd></column></table></schema></tableset></ri:Resource>