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<ri:Resource created="2010-11-23T07:51:45Z" 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>Radio evolution of the PN NGC 7027</title><shortName>J/ApJ/681/1296</shortName><identifier>ivo://CDS.VizieR/J/ApJ/681/1296</identifier><altIdentifier>doi:10.26093/cds/vizier.16811296</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zijlstra A.A.</name></creator><creator><name>van Hoof P.A.M.</name></creator><creator><name>Perley R.A.</name></creator><date role="Updated">2010-12-06T11:26:56Z</date><date role="Created">2010-11-23T07:51:45Z</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>planetary-nebulae</subject><subject>radio-continuum-emission</subject><description>We present the results of a 25yr program to monitor the radio flux evolution of the planetary nebula NGC 7027. We find significant evolution of the spectral flux densities. The flux density at 1465MHz, where the nebula is optically thick, is increasing at a rate of 0.251+/-0.015%/yr, caused by the expansion of the ionized nebula. At frequencies where the emission is optically thin, the spectral flux density is changing at a rate of -0.145+/-0.005%/yr, caused by a decrease in the number of ionizing photons coming from the central star. A distance of 980+/-100pc is derived. By fitting interpolated models of post-AGB evolution to the observed changes, we find that over the 25yr monitoring period, the stellar temperature has increased by 3900+/-900K and the stellar bolometric luminosity has decreased by 1.75+/-0.5%. We derive a distance-independent stellar mass of 0.655+/-0.010M_{sun}_ adopting the Blocker stellar evolution models, or about 0.04M_{sun}_ higher when using models of Vassiliadis &amp; Wood. A Cloudy photoionization model is used to fit all epochs at all frequencies simultaneously. The differences between the radio flux density predictions and the observed values show some time-independent residuals of typically 1%. A possible explanation is inaccuracies in the radio flux scale of Baars and coworkers. We propose an adjustment to the flux density scale of the primary radio flux calibrator 3C 286, based on the Cloudy model of NGC 7027. We also calculate precise flux densities for NGC 7027 for all standard continuum bands used at the VLA, as well as for some new 30 GHz experiments.</description><source format="bibcode">2008ApJ...681.1296Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/681/1296</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/442/249">J/A+A/442/249 : Integrated spectrum of NGC 7027 (Zhang+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/303/175">J/A+A/303/175 : Line spectrum of NGC 7027 (Baluteau+, 1995)</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/681/1296</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/681/1296</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/681/1296</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/681/1296</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/681/1296</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/681/1296</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>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/681/1296/table6</name><description>Model flux densities for NGC 7027</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>Freq</name><description>Frequency</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>NGC 7027 model flux density for epoch 2000.0</description><unit>mJy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SecVar</name><description>Secular variation of the flux density</description><unit>mJy/yr</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/681/1296/table1</name><description>*NGC 7027/3C 286 flux density ratios, with uncertainties</description><column><name>R8435</name><description>? NGC 7027/3C 286 flux density ratio at 8435MHz</description><ucd>phot.flux.density;em.radio.6-12GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></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>Epoch</name><description>Epoch (in decimal years)</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R1275</name><description>? NGC 7027/3C 286 flux density ratio at 1275MHz</description><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_R1275</name><description>? R1275MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>R1465</name><description>NGC 7027/3C 286 flux density ratio at 1465MHz</description><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_R1465</name><description>R1465MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R4535</name><description>? NGC 7027/3C 286 flux density ratio at 4535MHz</description><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_R4535</name><description>? R4535MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R4885</name><description>NGC 7027/3C 286 flux density ratio at 4885MHz</description><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R4885</name><description>R4885MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R8435</name><description>? R8435MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R8735</name><description>? NGC 7027/3C 286 flux density ratio at 8735MHz</description><ucd>phot.flux.density;em.radio.6-12GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_R8735</name><description>? R8735MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R14965</name><description>NGC 7027/3C 286 flux density ratio at 14965MHz</description><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R14965</name><description>R14965MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R22460</name><description>NGC 7027/3C 286 flux density ratio at 22460MHz</description><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R22460</name><description>R22460MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R43340</name><description>? NGC 7027/3C 286 flux density ratio at 43340MHz</description><ucd>phot.flux.density;em.mm.30-50GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_R43340</name><description>? R43340MHz uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>