Evolution of the compact radio source 3C 345.
Abstract
The quasar 3C 345 is recognized as a strong, variable, superluminal radio source, an optically violent variable, and a weak X-ray source. The authors present results of VLBI monitoring between 1979 and 1984 at 2.3, 5.0, 10.7, and 22.2 GHz. These results are interpreted in terms of a relativistic jet model.
- Publication:
-
Quasars
- Pub Date:
- 1986
- Bibcode:
- 1986IAUS..119..157B
- Keywords:
-
- Jets:Quasars;
- Quasars:Evolution;
- Quasars:Jets;
- Quasars:Superluminal Motions;
- Superluminal Motions:Quasars