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<ri:Resource created="2023-03-20T15:40:15Z" 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>Ultra-wideband (0.4-4GHz) study of CU Vir</title><shortName>J/ApJ/921/9</shortName><identifier>ivo://CDS.VizieR/J/ApJ/921/9</identifier><altIdentifier>doi:10.26093/cds/vizier.19210009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Das B.</name></creator><creator><name>Chandra P.</name></creator><date role="Updated">2023-07-03T14:36:38Z</date><date role="Created">2023-03-20T15:40:15Z</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>peculiar-variable-stars</subject><subject>radio-astronomy</subject><subject>polarimetry</subject><description>The presence of a large-scale surface magnetic field in early-type stars leads to several unique electromagnetic phenomena producing radiation over X-ray to radio bands. Among them, the rarest type of emission is electron cyclotron maser emission (ECME) observed as periodic, circularly polarized radio pulses. The phenomenon was first discovered in the hot magnetic star CU Vir. Past observations of this star led to the consensus that the star produces only right circularly polarized ECME, suggesting that only one magnetic hemisphere takes part in the phenomenon. Here we present the first ultra-wideband (0.4-4GHz) study of this star using the upgraded Giant Metrewave Radio telescope and the Karl G. Jansky Very Large Array, which led to the surprising discovery of ECME of both circular polarizations up to around 1.5GHz. The GHz observations also allowed us to infer that the upper ECME cutoff frequency is at &gt;=5GHz. The sub-GHz observation led to the unexpected observation of more than two pairs of ECME pulses per rotation cycle. In addition, we report the discovery of a "giant pulse" and transient enhancements, which are potentially the first observational evidence of "centrifugal breakout" of plasma from the innermost part of the stellar magnetosphere. The stark contrast between the star's behavior at GHz and sub-GHz frequencies could either be due to propagation effects, a manifestation of varying magnetic field topology as a function of height, or a signature of an additional "ECME engine."</description><source format="bibcode">2021ApJ...921....9D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/921/9</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/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/polarbase">B/polarbase : PolarBase spectropol. database (ESPaDOnS, NARVAL) (Petit+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/117/335">J/A+AS/117/335 : Optical positions of radio emitting stars (Assafin+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/130/215">J/A+AS/130/215 : Effective temperatures of Ap stars (Sokolov, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/383/1062">J/A+A/383/1062 : Opt. positions of 55 radio stars at Yunnan Obs. (Hu+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/931">J/A+A/493/931 : MAD observations of {sigma} Ori (Bouy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/2106">J/MNRAS/431/2106 : CU Vir Stroemgren differential photometry (Pyper+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/2240">J/MNRAS/431/2240 : Activity in A-type stars from Kepler (Balona, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/126/469">J/PASP/126/469 : PolarBase catalogue of stellar spectra (Petit+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/A34">J/A+A/625/A34 : Photometry of CU Vir (Krticka+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/499/5379">J/MNRAS/499/5379 : Longitudinal magnetic field of 6 B stars (Shultz+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/504/3730">J/MNRAS/504/3730 : Synthetic RGB photometry of bright stars (Cardiel+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/652/A31">J/A+A/652/A31 : Stellar magnetic rot. phase curves. II (Bychkov+, 2021)</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/921/9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/921/9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/921/9</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/921/9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/921/9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/921/9</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/921/9/fluxes</name><description>Flux density measurements at uGMRT band 3 (300-500MHz) and band 4 (550-900MHz) and at VLA L band (1000-2000MHz) and S band (2000-4000MHz), tables 2-5</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>HJD1</name><description>Heliocentric Julian Day, observation start</description><unit>d</unit><ucd>time.start;obs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>HJD2</name><description>Heliocentric Julian Day, observation end</description><unit>d</unit><ucd>time.end;obs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[-1.9/184] Flux density in Band</description><unit>mJy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>[0.2/19] Uncertainty in Flux (1)</description><unit>mJy</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pol</name><description>Polarization type ("RCP"; "LCP") (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>nu0</name><description>[347/3947] Central frequency of a band</description><unit>MHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dnu</name><description>[22/1128] Bandwidth</description><unit>MHz</unit><ucd>instr.bandwidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Band</name><description>uGMRT (3=300-500MHz; 4=550-900MHz) or VLA (L=1-2GHz; S=2-4GHz) observation band</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>