Millimeter and submillimeter polarization observations of blazars from the James Clerk Maxwell Telescope are presented. The data are interpreted in light of recent results from centimeter wavelength VLBI polarimetry studies. Observations of the superluminal quasar 3C 279 at 1.1 and 0.8 mm give a degree of polarization in excess of 10% and imply that the magnetic field is aligned orthogonal to the milliarcsecond (mas) jet to within 6°. This magnetic field orientation is consistent with that expected to arise in a transverse shock. The high level of polarization suggests that the centimeter VLBI core is depolarized by Faraday rotation rather than by increased magnetic field disorder at the base of the inhomogeneous relativistic jet. Three BL ...
We review results from the POLAMI program, which monitors the polarization properties of 36 blazars ...
The gamma-ray blazar 1611+343 was observed with polarization VLBI mode at 5 GHz in February 1999. Th...
We report preliminary results of a 3-year multifrequency polarization campaign of 15 AGNs of blazar ...
We present 43 GHz polarization images obtained with the Very Long Baseline Array of four blazars (08...
We present 43 GHz polarization images obtained with the Very Long Baseline Array of four blazars (08...
We are engaged in a long-term project to monitor the polarized intensity structure of 15 blazars (in...
We report on preliminary results from the first monitoring campaign of the submillimetre polarizatio...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronom...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
The high radio frequency polarization imaging of non-thermal emission from active galactic nuclei (A...
e are engaged in a long-term project to monitor the polarized intensity structure of 15 blazars and ...
The results of intensive multiwavelength observations of a sample of 19 blazars reveal a distinct co...
We report results from a deep polarization imaging of the nearby radio galaxy 3C 84 (NGC 1275). The ...
We review results from the POLAMI program, which monitors the polarization properties of 36 blazars ...
The gamma-ray blazar 1611+343 was observed with polarization VLBI mode at 5 GHz in February 1999. Th...
We report preliminary results of a 3-year multifrequency polarization campaign of 15 AGNs of blazar ...
We present 43 GHz polarization images obtained with the Very Long Baseline Array of four blazars (08...
We present 43 GHz polarization images obtained with the Very Long Baseline Array of four blazars (08...
We are engaged in a long-term project to monitor the polarized intensity structure of 15 blazars (in...
We report on preliminary results from the first monitoring campaign of the submillimetre polarizatio...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronom...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
The high radio frequency polarization imaging of non-thermal emission from active galactic nuclei (A...
e are engaged in a long-term project to monitor the polarized intensity structure of 15 blazars and ...
The results of intensive multiwavelength observations of a sample of 19 blazars reveal a distinct co...
We report results from a deep polarization imaging of the nearby radio galaxy 3C 84 (NGC 1275). The ...
We review results from the POLAMI program, which monitors the polarization properties of 36 blazars ...
The gamma-ray blazar 1611+343 was observed with polarization VLBI mode at 5 GHz in February 1999. Th...
We report preliminary results of a 3-year multifrequency polarization campaign of 15 AGNs of blazar ...