Superluminal Motion in the Large, Strongly Lobe-dominated Quasar 3C 47

Details Superluminal Motion in the Large, Strongly Lobe-dominated Quasar 3C 47 Superluminal Motion in the Large, Strongly Lobe-dominated Quasar 3C 47

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...417..541v&link_type=abstract

Astrophysical Journal v.417, p.541

Astronomy and Astrophysics

Astronomy

16

Galaxies: Jets, Galaxies: Quasars: Individual Alphanumeric: 3C 47, Radio Continuum: Galaxies

Scientific paper

Dual-epoch 10.7 GHz VLBI observations of the large, lobe-dominated quasar 3C 47 reveal a component moving with an apparent transverse velocity of (3.7+0.9-0.7) h-1c (with H0 = 100 h km s-1 Mpc-1, q0 = 0.5). 3C 47 is the most strongly lobe-dominated superluminal found to date, and it has the largest projected linear extent in our complete, low-frequency selected sample. Its moderately large superluminal motion is difficult to understand in the light of simple relativistic beaming models and popular unification hypotheses.

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