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<ri:Resource created="2019-08-14T13:44:12Z" 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>Rotation reversals in the polarization in OJ 287</title><shortName>J/ApJ/862/1</shortName><identifier>ivo://CDS.VizieR/J/ApJ/862/1</identifier><altIdentifier>doi:10.26093/cds/vizier.18620001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cohen M.H.</name></creator><creator><name>Aller H.D.</name></creator><creator><name>Aller M.F.</name></creator><creator><name>Hovatta T.</name></creator><creator><name>Kharb P.</name></creator><creator><name>Kovalev Y.Y.,Lister M.L.</name></creator><creator><name>Meier D.L.</name></creator><creator><name>Pushkarev A.B.</name></creator><creator><name>Savolainen T.</name></creator><date role="Updated">2019-11-27T11:28:09Z</date><date role="Created">2019-08-14T13:44:12Z</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>polarimetry</subject><subject>bl-lacertae-objects</subject><subject>radio-continuum-emission</subject><description>We have obtained a smooth time series for the electric vector position angle (EVPA) of the blazar OJ 287 at centimeter wavelengths, by making +/-n{pi} adjustments to archival values from 1974 to 2016. The data display rotation reversals in which the EVPA rotates counterclockwise for ~180{deg} and then rotates clockwise by a similar amount. The timescale of the rotations is a few weeks to a year, and the scale for a double rotation, including the reversal, is 1-3yr. We have seen four of these events in 40yr. A model consisting of two successive outbursts in polarized flux density, with EVPAs counterrotating, superposed on a steady polarized jet, can explain many of the details of the observations. Polarization images support this interpretation. The model can also help to explain similar events seen at optical wavelengths. The outbursts needed for the model can be generated by the supermagnetosonic jet model of Nakamura+ (2010ApJ...721.1783N) and Nakamura &amp; Meier (2014ApJ...785..152N), which requires a strong helical magnetic field. This model produces forward and reverse pairs of fast and slow MHD waves, and the plasma inside the two fast/slow pairs rotates around the jet axis, but in opposite directions.</description><source format="bibcode">2018ApJ...862....1C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/862/1</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+AS/39/379">J/A+AS/39/379 : Linear Polarization of radio sources (Tabara+ 1980)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/87/859">J/AJ/87/859 : Polarisation of 404 radio sources at 6 and 20cm (Perley, 1982)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/129/569">J/A+AS/129/569 : BVRI photometry of OJ 287 (Jia Guibin+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/139/545">J/A+AS/139/545 : 1-22 GHz spectra survey (Kovalev+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/522/846">J/ApJ/522/846 : Optical monitoring of GeV loud blazars (Xie+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/441/915">J/A+A/441/915 : Alignments of quasar polarization vectors (Hutsemekers+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1418">J/AJ/130/1418 : AGN jet kinematics (Jorstad+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1389">J/AJ/130/1389 : Linear polarization of AGN jets at 15GHz (Lister+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1262">J/AJ/131/1262 : Circ. polarization images at 15GHz of AGN jets (Homan+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1256">J/AJ/132/1256 : eim BATC photometry of OJ 287 (Wu+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1947">J/AJ/133/1947 : 37GHz observations of BL Lac objects (Nieppola+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/799">J/AJ/134/799 : Multiwaveband polarimetry of 15 AGN (Jorstad+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/380/162">J/MNRAS/380/162 : Aligned radio polarizations of quasars (Joshi+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/385/823">J/MNRAS/385/823 : UBVRI light curves of OJ 287 (Zheng+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3718">J/AJ/137/3718 : 15GHz monitoring of AGN jets with VLBA (Lister+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/402/2087">J/MNRAS/402/2087 : Opt. polarization of OJ 287 in 2005-2009 (Villforth+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/189/1">J/ApJS/189/1 : A 3.5mm polarimetric survey of radio-loud AGNs (Agudo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/19">J/ApJS/194/19 : Optical linear polarization at McDonald Obs. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Date</name><description>[1971.3/2012.5] Observation epoch, fractional year</description><unit>yr</unit><ucd>time.epoch;obs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>nu</name><description>[4.8/14.5] Observation frequency</description><unit>GHz</unit><ucd>em.freq;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ftot</name><description>[1/10.4] Total flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pol</name><description>[0.4/17.5] Fractional linear polarization</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EVPA</name><description>[-1000/202.5] Adjusted electric vector position angle</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/862/1/table2</name><description>MOJAVE 15GHz VLBA core feature data</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>Date</name><description>[1996/2015.6] Observation epoch, fractional year</description><unit>yr</unit><ucd>time.epoch;obs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>I</name><description>[0.86/5.96] Stokes I intensity</description><unit>Jy/beam</unit><ucd>phys.polarization.stokes</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pol</name><description>[0.2/10.8] Fractional linear polarization</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EVPA</name><description>[-90/198] Adjusted electric vector position angle</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/ApJ/862/1/table3</name><description>Kikuchi+ (1988A&amp;A...190L...8K) 10GHz radio data</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>Date</name><description>[1986/1986.5] Observation Epoch, fractional year</description><unit>yr</unit><ucd>time.epoch;obs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ftot</name><description>[0.2/2.7]? Total flux density at 10GHz</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.6-12GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pol</name><description>[3.5/7.2]? Fractional linear polarization</description><unit>%</unit><ucd>phys.polarization.linear</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EVPA</name><description>[-206/108]? Adjusted electric vector position angle</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>