Superluminal Radio Source PKS 0420-014

Details Superluminal Radio Source PKS 0420-014 Superluminal Radio Source PKS 0420-014

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998chphl..15..545h&link_type=abstract

Chinese Physics Letters, Volume 15, Issue 7, pp. 545-546 (1998).

Physics

9

Scientific paper

The very long baseline interferometry result of a superluminal radio source PKS 0420-014 at 5 GHz with Shanghai (China), Urumqi (China), Noto (Italy), and HartRAO (South Africa) telescopes is presented. Proper motions of the relativistic jet components in the source are calculated. Based on the Self-Compton emission in a uniform spherical model, the beaming parameters of the source are estimated. The results show that PKS 0420-014 has a high Doppler factor of 9.3, a Lorentz factor of 6.5, and a small angle of 5.5° to the line of sight.

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