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Studies of the 3C 345 Quasar Structure at dm-Wavelengths
Published online by Cambridge University Press: 04 August 2017
Abstract
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The structure of the quasar 3C 345 has been studied at 18 and 49 cm wavelengths by VLBI method. The structure has a nucleus and a jet, which changes direction with distance from the nucleus. The continuum emission of the nucleus and the jet regions correspond to a source with a large optical depth, the cut frequence goes down with increasing distance from nucleus.
- Type
- V. Jets, Superluminal Motions and Blazars
- Information
- Symposium - International Astronomical Union , Volume 121: Observational Evidences of Activity of Galaxies , 1987 , pp. 301 - 304
- Copyright
- Copyright © Reidel 1987
References
Matveyenko, L.I., et al., Proc. VLBITTechniques Symp., Ed. Biraud F., Tolouse, 1982, 347.Google Scholar
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