Superluminal radio source PKS 0420-014


Autoria(s): Hong, XY; Jiang, DR; Shen, ZQ; Wan, TS
Data(s)

1998

Resumo

The very long baseline interferometry result of a superluminal radio source PKS 0420-014 at 5 GHz with Shanghai (China), Urumqi (China), Note (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 degrees to the line of sight.

Identificador

http://119.78.226.72//handle/331011/7919

http://www.irgrid.ac.cn/handle/1471x/82463

Idioma(s)

英语

Fonte

洪晓瑜;蒋栋荣;沈志强.Superluminal Radio Source PKS 0420-014,Chinese Physics Letters,1998,15(7):545

Palavras-Chave #射电天文学
Tipo

期刊论文