A Cocoon Transparency and the 3C 345 Low Frequency Variability

  • L. I. Matveenko
Conference paper
Part of the International Astronomical Union book series (IAUS, volume 175)

Abstract

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.

Keywords

Black Hole Brightness Temperature Position Angle Polarization Orientation Rotation Measure 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© International Astronomical Union 1996

Authors and Affiliations

  • L. I. Matveenko
    • 1
  1. 1.Space Research Institute of RASMoscowRussia

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