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<ri:Resource created="2022-10-28T09:37:49Z" 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>BVRI photometry of nova V5856 Sgr</title><shortName>J/A+A/667/A7</shortName><identifier>ivo://CDS.VizieR/J/A+A/667/A7</identifier><altIdentifier>doi:10.26093/cds/vizier.36670007</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Munari U.</name></creator><creator><name>Masetti N.</name></creator><creator><name>Walter F.M.</name></creator><creator><name>Williams R.E.</name></creator><creator><name>Hambsch F.-J.</name></creator><creator><name>Frigo A.,Valisa P.</name></creator><date role="Updated">2024-11-28T20:01:10Z</date><date role="Created">2022-10-28T09:37:49Z</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>novae</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>spectroscopy</subject><description>We report about the fast Nova Sgr 2016 N.4 being surprisingly trapped in a long-lasting and bright plateau (Delta(I)&gt;=10mag above quiescence), six years past the nova eruption. Very few other novae experience a similar occurring. We have carried out an intensive observing campaign collecting daily BVRI photometry, monthly high-resolution optical spectroscopy, and observed the nova in ultraviolet and X-rays with Swift at five distinct epochs. The bolometric luminosity radiated during the plateau is L(bol)~4200L_{sun}_ (scaled to the distance of the Galactic Bulge), corresponding to stable nuclear burning on a 0.6M_{sun}_ white dwarf. A stable wind is blown-off at FWZI~1600km/s, with episodic reinforcement of a faster FWZI~3400km/s mass-loss, probably oriented along the polar directions. The collision of such winds could power the emission detected in X-rays. The burning shell has an outer radius of ~25R_{sun}_ at which the effective temperature is ~7600K, values similar to those of a F0 II/Ib bright giant. The Delta(m)&lt;1mag variability displayed during the plateau is best described as chaotic, with the irregular appearance of quasi-periodic oscillations with a 15-17 days periodicity. A limited amount of dust (~3x10^-11^M_{sun}_) continuously condense at T(dust)~1200K in the outflowing wind, radiating L(dust)~52L_{sun}_.</description><source format="bibcode">2022A&amp;A...667A...7M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/667/A7</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/A+A/667/A7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/667/A7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/667/A7</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/667/A7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/667/A7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/667/A7</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><spectral>3.322582951404819e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/667/A7/table1</name><description>BVRI photometry of nova V5856 Sgr collected in 2021 and 2022</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>Heliocentric Julian date (HJD-2459000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Date</name><description>Date (UT) of the observation (YYYY-MM-DD.ddd)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Vmag</name><description>V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vmag</name><description>Error on Vmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-V</name><description>? B-V color</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_B-V</name><description>? Error on B-V color</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>V-R</name><description>? V-R color</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_V-R</name><description>? Error on V-R color</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R-I</name><description>? R-I color</description><unit>mag</unit><ucd>phot.color;em.opt.R;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_R-I</name><description>? Error on R-I color</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/667/A7/spectrum</name><description>Spectrum (fig. 2)</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>lambda</name><description>Heliocentric wavelength</description><unit>0.1nm</unit><ucd>em.wl;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Flux (in erg/cm^2^/s/{AA}</description><unit>10mW.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>