Helical motions in the jet of blazar 1156+295

Details Helical motions in the jet of blazar 1156+295 Helical motions in the jet of blazar 1156+295

1999-06-23

arxiv.org/abs/astro-ph/9906358v1

New Astron.Rev. 43 (1999) 699-702

Astronomy and Astrophysics

Astrophysics

6 pages, 2 figures, to appear in New Astronomy Reviews (EVN/JIVE Symposium No. 4, special issue)

Scientific paper

10.1016/S1387-6473(99)00081-0

The blazar 1156+295 was observed by VLBA and EVN + MERLIN at 5 GHz in June 1996 and February 1997 respectively. The results show that the jet of the source has structural oscillations on the milliarcsecond scale and turns through a large angle to the direction of the arcsecond-scale extension. A helical jet model can explain most of the observed properties of the radio structure in 1156+295.

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