Superluminal motion in the giant quasar 4C 34.47

Details Superluminal motion in the giant quasar 4C 34.47 Superluminal motion in the giant quasar 4C 34.47

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336..601b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 15, 1989, p. 601-605.

Astronomy and Astrophysics

Astrophysics

44

Extragalactic Radio Sources, Quasars, Luminosity, Relativistic Electron Beams, Very Long Base Interferometry

Scientific paper

Superluminal motion in the core of 4C 34.47, the largest radio source associated with a QSO, has been detected. The data indicate an apparent superluminal core expansion speed of (2.5 + or - 0.2/h c(h0 = 100h km/s Mpc and q0 = 0.5). The superluminally expanding core of 4C 34.47 is embedded in a double-lobed radio source which is extended by 560/h kpc. Explanation of the superluminal character of 4C 34.47 in the framework of relativistic beaming is considered.

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