Are 3C 249.1 and 3C 334 restarted quasars?
Toruń Centre for Astronomy, N. Copernicus University, 87-100 Toruń, Poland
Received: 13 July 2012
Accepted: 23 August 2012
This Research Note follows up a Letter in which I posit that J1211+743 is a restarted radio source. This means that its structure, where the jet points to the relic lobe, is only apparently paradoxical. Here, I propose the same scenario and apply the same mathematical model to 3C 249.1 and 3C 334. The ultimate result of my investigation is that these two well-known radio-loud quasars can be understood best so far if it was assumed that they, too, had been restarted.
Key words: radio continuum: galaxies / galaxies: active
© ESO, 2012