Theoretical properties of radio-galaxies. II - Luminosity and energetics

Details Theoretical properties of radio-galaxies. II - Luminosity and energetics Theoretical properties of radio-galaxies. II - Luminosity and energetics

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.109..287z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 109, no. 2, Feb. 1985, p. 287-292.

Astronomy and Astrophysics

Astrophysics

1

Galactic Radio Waves, Luminosity, Radio Galaxies, Accretion Disks, Density Distribution, Mass Flow, Turbulence

Scientific paper

Using the turbulent cascade approach, the theoretical luminosity of a radio-galaxy is deduced and compared with the observed luminosity from a large sample of symmetric double radio-galaxies. By equalizing the two luminosities, the density and energetics function of the intrinsic radio-luminosities are obtained. Consideration is given to the determination of the mass and energy outflow in external regions and in VBLI-jets, and to the product of velocity and density in the pc region of a thick accretion disk.

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