Properties of the extended lobes of radio galaxies and quasars in the framework of the "flip-flop" model

Details Properties of the extended lobes of radio galaxies and quasars in the framework of the "flip-flop" model Properties of the extended lobes of radio galaxies and quasars in the framework of the "flip-flop" model

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..135z&link_type=abstract

Astronomy Reports, Volume 43, Issue 3, March 1999, pp.135-141

Astronomy and Astrophysics

Astronomy

3

Scientific paper

The observed asymmetry of the radio images of double-lobed quasars in the 3CR and 4C surveys is examined as a function of their radio luminosity. Theoretical models explaining various aspects of this asymmetry discussed earlier in the literature are considered. The observational data can be explained using a "flip-flop" model with certain relationships between temporal parameters. In this case, the number of times the radio jet has changed direction increases from three for quasars with radio luminosities P > 10^28 W/Hz to five for quasars with P < 10^28 W/Hz. Some peculiarities of the structures of radio sources are discussed in the framework of this flip-flop model.

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