Superluminal motion in AGN (Zhang+, 2008)

Details Superluminal motion in AGN (Zhang+, 2008) Superluminal motion in AGN (Zhang+, 2008)

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycatp028000801z&link_type=abstract

VizieR On-line Data Catalog: J/other/ChJAA/8.385. Originally published in: 2008ChJAA...8..385Z

Other

Active Gal. Nuclei, Bl Lac Objects, Qsos, Proper Motions, Redshifts

Scientific paper

We have collected an up-to-date sample of 123 superluminal sources (84 quasars, 27 BL Lac objects and 12 galaxies) and calculated the apparent velocities (βapp) for 224 components in the sources with the Λ-CDM model. We checked the relationships between their proper motions, redshifts, βapp and 5GHz flux densities. Our analysis shows that the radio emission is strongly boosted by the Doppler effect. The superluminal motion and the relativistic beaming boosting effect are, to some extent, the same in active galactic nuclei.
(2 data files).

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