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Time-Variable Faraday Rotation Measures of 3C 273 and 3C 279
Author(s) -
R. T. Zavala,
G. B. Taylor
Publication year - 2001
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/319653
Subject(s) - physics , faraday effect , quasar , position angle , polarimetry , astrophysics , line of sight , rotation (mathematics) , faraday cage , very long baseline array , optics , magnetic field , scattering , galaxy , geometry , mathematics , quantum mechanics
Multifrequency polarimetry with the VLBA confirms the previously reportedtime-varying Faraday rotation measure (RM) in the quasar 3C-279. Variability inthe RM and electric vector position angle (EVPA) of the jet component (C4) isseen making it an unreliable absolute EVPA calibrator. 3C-273 is also shown tovary its RM structure on 1.5 year time-scales. Variation in the RM propertiesof quasars may result from a Faraday screen which changes on time-scales of afew years, or from the motion of jet components which sample spatial variationsin the screen. A new component emerging from the core of 3C-279 appears to bestarting to sample such a spatial variation. Future monitoring of thiscomponent and its RM properties is suggested as a diagnostic of the narrow lineregion in 3C-279. We also present a new method of EVPA calibration using theVLA Monitoring Program.Comment: Accepted to ApJ Letters. 12 pages, 5 figure

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