Is 0716 + 714 a superluminal blazar ?
نویسندگان
چکیده
We present an analysis of new and old high frequency VLBI data collected during the last 10 years at 5– 22 GHz. For the jet components in the mas-VLBI jet, two component identifications are possible. One of them with quasi-stationary components oscillating about their mean positions. Another identification scheme, which formally gives the better expansion fit, yields motion with ∼ 9 c for H0 = 65 km s −1 Mpc −1 and q0 = 0.5. This model would be in better agreement with the observed rapid IDV and the expected high Lorentz-factor, deduced from IDV.
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