The superluminal source 0106+013.

Details The superluminal source 0106+013. The superluminal source 0106+013.

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acaps..17..126s&link_type=abstract

Acta Astrophys. Sin., Vol. 17, No. 2, p. 126 - 128

Astronomy and Astrophysics

Astrophysics

Radio Sources: Superluminal Motions, Radio Sources: Vlb Interferometry

Scientific paper

The authors observed 0106+013 with a VLBI array of SHEVE plus Shanghai at 5 GHz. The results show that (1) the component 1 is most likely the core, (2) the original superluminal component is still moving outwards at a speed of 0.2 mas/yr, (3) a new component emerging from the core is moving outwards at a speed of 0.18 mas/yr, and (4) the jet bends within 5 mas of the core and then extends along the VLA jet.

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