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Superluminal Radio Source PKS 0420-014 |
| HONG Xiao-yu;JIANG Dong-rong;SHEN Zhi-qiang;WAN Tong-shan |
| Shanghai Observatory, Chinese Academy of Sciences, Shanghai 200030 |
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| Cite this article: |
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HONG Xiao-yu, JIANG Dong-rong, SHEN Zhi-qiang et al 1998 Chin. Phys. Lett. 15 545-546 |
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Abstract 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 5.5º to the line of sight.
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| Keywords:
98.54.Cm
95.85.Te
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Published: 01 July 1998
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| PACS: |
98.54.Cm
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(Active and peculiar galaxies and related systems (including BL Lacertae objects, blazars, Seyfert galaxies, Markarian galaxies, and active galactic nuclei))
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95.85.Te
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