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A Cocoon Transparency and the 3C 345 Low Frequency Variability
Published online by Cambridge University Press: 25 May 2016
Abstract
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The structure of the quasar 3C 345 is studied at λ = 49cm. The core has a low-frequency cut off spectrum and α ≃ 3. The brightest knot is in the nearest part of the jet. The cocoon wall absorbs low-frequency emission and changes the polarization orientation, RM = 3500 rad m –2, B|| ≃ 100 μG at the core region.
- Type
- Radio Source Modelling and Emission Mechanisms
- Information
- Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 485 - 486
- Copyright
- Copyright © Kluwer 1996
References
1. Matveenko, L.I., Graham, D.A., Pauliny-Toth, I.I.K., et al. (1992)
Pis'ma v Astron. Zh.
, Vol. 18, p 931
Google Scholar
2. Matveenko, L.I., Pauliny-Toth, I.I.K., Baath, L.B., et al. (1996)
Pis'ma v Astron. Zh.
, Vol. 22, p in press
Google Scholar
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