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Circular Polarization Variability in Extragalactic Sources on Time Scales of Months to Decades

dc.contributor.authorAller, Hugh D.en_US
dc.contributor.authorAller, Margo F.en_US
dc.contributor.authorPlotkin, Richard M.en_US
dc.date.accessioned2006-09-08T19:52:11Z
dc.date.available2006-09-08T19:52:11Z
dc.date.issued2003-03en_US
dc.identifier.citationAller, Hugh D.; Aller, Margo F.; Plotkin, Richard M.; (2003). "Circular Polarization Variability in Extragalactic Sources on Time Scales of Months to Decades." Astrophysics and Space Science 288 (1-2): 17-28. <http://hdl.handle.net/2027.42/42005>en_US
dc.identifier.issn0004-640Xen_US
dc.identifier.issn1572-946Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/42005
dc.description.abstractWe present previously unpublished circular polarization (cp) measurementsat 4.8 and 8.0 GHz made with the University of Michigan 26-meter primefocus telescope during 1978–1984 and results of a newobservational program during the past two years. Based on the preliminary analysis of our recent data, eight sources were detected at 4.8 GHz with average degrees of cp ranging from ≤ 0.1% to ≥ 1%.The results are compared with observations at other frequencies and with linearpolarization and total flux density variability in the sources.The behavior of the cp variability observed to date is consistentwith stochastic variations produced by mode conversion in transient,opaque emitting regions in the sources. The observed sign changes observedbetween different epochs and different frequencies are not consistentwith the hypothesis that sources maintain a fixed handedness of cp.en_US
dc.format.extent501902 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.subject.otherCircular Polarizationen_US
dc.subject.otherVariabilityen_US
dc.titleCircular Polarization Variability in Extragalactic Sources on Time Scales of Months to Decadesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, USAen_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, USAen_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/42005/1/10509_2004_Article_5252793.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/B:ASTR.0000004990.22510.53en_US
dc.identifier.sourceAstrophysics and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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