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Multiband Photopolarimetric Monitoring of an Outburst of the Blazar 3C 454.3 in 2007

机译:2007年Blazar 3C 454.3爆发的多波段光极化监测

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Wereportonopticala€”near-infraredphotopolarimetricobservationsofablazar3C454.3over200d.Theobjectexperiencedanopticaloutburstin2007July.Thisoutburstwasfollowedbyashortstatefainterthan$$V=$$15.2mag,lasting$$sim$$25d.Theobjectthenenteredanactivestateduringwhichweobservedshortflareshavingatimescaleof3a€“10d.Theobjectshowedtwotypesoffeaturesinthecolora€“magnituderelationship.Onewasaa€?bluer-when-brightera€?trendintheoutburststate,andtheotherwasaa€?redder-when-brightera€?trendinthefaintstate.Thesetwotypesoffeaturessuggestacontributionofthermalemissiontotheobservedflux,assuspectedinpreviousstudies.Ourpolarimetricobservationdetectedtwoepisodesofrotationofthepolarizationvector.Thefirstonewasacounterclockwiserotationinthe$$QU$$planeduringtheoutburststate.Afterthisrotationeventofthepolarizationvector,theobjectenteredarapidlyfadingstage.Thesecondonewasseeninaseriesofflaresduringtheactivestate.Eachflarehadaspecificpositionangleofpolarization,whichapparentlyrotatedclockwisefromthefirsttothelastflares.Thus,theobjectexhibitedrotationsofthepolarizationvectorinoppositedirections.Weestimatedadecaytimescaleoftheshortflaresduringtheactivestate,andthencalculatedanupperlimitofthestrengthofthemagneticfield,$$B=$$0.2G,assumingatypicalbeamingfactorofblazars,$$delta=$$20.Thisupperlimitof$$B$$issmallerthanthosepreviouslyestimatedfromspectralanalysis.
机译:Wereportonopticala€”近infraredphotopolarimetricobservationsofablazar3C454.3over200d.Theobjectexperiencedanopticaloutburstin2007July.Thisoutburstwasfollowedbyashortstatefainterthan $$ V = $$ 15.2mag,持久$$ SIM $$ 25d.Theobjectthenenteredanactivestateduringwhichweobservedshortflareshavingatimescaleof3a€“10d.Theobjectshowedtwotypesoffeaturesinthecolora€“magnituderelationship.Onewasaa€?更蓝 - 当 - 的BrightEra€?trendintheoutburststate, andtheotherwasaa€?更红 - 当 - 的BrightEra€?trendinthefaintstate.Thesetwotypesoffeaturessuggestacontributionofthermalemissiontotheobservedflux,assuspectedinpreviousstudies.Ourpolarimetricobservationdetectedtwoepisodesofrotationofthepolarizationvector.Thefirstonewasacounterclockwiserotationinthe $$曲$$ planeduringtheoutburststate.Afterthisrotationeventofthepolarizationvector,theobjectenteredarapidlyfadingstage.Thesecondonewasseeninaseriesofflaresduringtheactivestate.Eachflarehadaspecificpositionangleofpolarization,whichapparentlyrotatedclockwisefromthefirsttothelastflare因此,物体在相反方向上表现出极化矢量的旋转。我们估算了在活动状态期间短喇叭形的大约时间尺度,然后计算出磁场强度的上限,$ B = $ 0.2G,假设该误差是典型的上限,则$$ delta = $ 20的原假设。

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