The separation velocity of radio components in QSO

Details The separation velocity of radio components in QSO The separation velocity of radio components in QSO

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977acasn..18..239y&link_type=abstract

Acta Astronomica Sinica, vol. 18, Dec. 1977, p. 239-247. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

1

Luminous Intensity, Quasars, Radiant Flux Density, Radio Emission, Relativistic Velocity, Radio Sources (Astronomy), Relativistic Effects, Statistical Distributions

Scientific paper

For QSO with double radio components, the separation velocity of the components with respect to the optical parent body can be derived from the radio flux ratio of the two components and the evolution law of radio luminosity. The observational data of 26 samples have been analyzed, and the following results obtained: the separation velocity is within the range 0.2-0.14 c, the average velocity is about 0.09 c and the upper limit of the initial eruption velocity is about 0.35 c.

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