Theoretical parameters of powerful radio galaxies - Hydrodynamic approximation

Details Theoretical parameters of powerful radio galaxies - Hydrodynamic approximation Theoretical parameters of powerful radio galaxies - Hydrodynamic approximation

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....25..369b&link_type=abstract

(Astrofizika, vol. 25, Sept.-Oct. 1986, p. 369-381) Astrophysics (ISSN 0571-7132), vol. 25, no. 2, March 1987, p. 569-576. Trans

Statistics

Computation

1

Computational Astrophysics, Extragalactic Radio Sources, Hydrodynamic Equations, Plasma Interactions, Plasma Jets, Radio Galaxies, Interstellar Gas, Interstellar Magnetic Fields, Kinetic Energy, Shock Wave Propagation

Scientific paper

The basic physical parameters of a characteristic 3C FR II radio source are estimated. The statistical relationships between the velocity, density, mass flux of the jet, and the luminosity of the hotspot are predicted. The obtained estimates indicate a high efficiency of transformation of the kinetic energy of the jet into the energy of ultrarelativistic particles, magnetic fields, and synchrotron radiation.

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