Jorstad, S. G., Marscher, A. P., Stevens, J. A., Robson, E. I., Lister, J. L., Stirling, A. M., Smith, P. S., Cawthorne, T. V., Gomez, J. L., Gabuzda, D. C. and Gear, Walter Kieran ORCID: https://orcid.org/0000-0001-6789-6196 2005. Multi-frequency polarization properties of Blazars. Presented at: Astronomical Polarimetry: Current Status and Future Directions, Waikoloa, HI, USA, 15-19 March 2004. Published in: Adamson, Andy, Aspin, Colin, Davis, Chris J. and Fujiyoshi, Takuya eds. Astronomical Polarimetry: Current Status and Future Directions. ASP Conference Series (343) San Francisco, CA: Astronomical Society of the Pacific, pp. 469-473. |
Abstract
We have obtained total and polarized intensity images of 15 AGNs with the VLBA at 7 mm at 17 epochs, accompanied at many epochs by nearly simultaneous measurements of polarization at 1.35/0.85 mm and at optical wavelengths. Analysis of the data shows an obvious connection between the polarized emission at high frequencies and the most strongly polarized features in parsec-scale jets. The largest deviations between polarization parameters at different frequencies are detected when a new compact knot emerges from the core, and are likely caused by very short time-scale (<1 week) polarization variability during the events.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy Neuroscience and Mental Health Research Institute (NMHRI) |
Subjects: | Q Science > QB Astronomy |
Additional Information: | Proceedings of conference held at Waikoloa, Island of Hawaii, Hawaii, USA 15-19 March 2004 |
Publisher: | Astronomical Society of the Pacific |
ISBN: | 1583812105 |
Related URLs: | |
Last Modified: | 21 Oct 2022 09:27 |
URI: | https://orca.cardiff.ac.uk/id/eprint/36550 |
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