Observations of the superluminal source 0106+013

Details Observations of the superluminal source 0106+013 Observations of the superluminal source 0106+013

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..265s&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 21, Issue 3, p. 265-268.

Astronomy and Astrophysics

Astrophysics

Scientific paper

In the course of a Southern Sky, 5 GHz VLBI Survey using the Shanghai+SHEVE network, we made further studies on the superluminal motion of the compact radio source 0106+013. The results show 1) that Component 1 is most likely to be the core, 2) that the original superluminal jet is continuing to move outward at a proper motion of 0.2 mas/yr, 3) the explosion of a new component which is again superluminal at a proper motion of 0.18 mas/yr and 4) that the jet shows clear bending at about 5 mas and then tends to the direction of the VLA jet.

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