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OJ 287 as a Rotating Helix.

Authors :
Cohen, Marshall H.
Source :
Galaxies (2075-4434); 2017, Vol. 5 Issue 1, p12, 8p
Publication Year :
2017

Abstract

We present preliminary data from high-cadence 15-GHz VLBA images of OJ 287 from 1995 to 2015. The ridgelines suggest that the jet is rotating, perhaps with a period of 30 years. The EVPA of the core rotated by 240° in 2001-2002 and decreased slowly after that. The inner jet apparently moved to a new direction after the rotation, as shown by the emergence of a new component at a new PA at 43 GHz, in 2004. This was presaged by a strong rise in the flux density of the core, and then its sudden fall as the new component was identified. The equivalent sequence of events took place about 5 years later at 15 GHz, but in addition the core EVPA had a step in 2006 and moved to be aligned with the new 43-GHz component. The 15-GHz core became optically thin in 2006, but the angular resolution was insufficient to separate the new component from the core until 2010. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
20754434
Volume :
5
Issue :
1
Database :
Complementary Index
Journal :
Galaxies (2075-4434)
Publication Type :
Academic Journal
Accession number :
122322382
Full Text :
https://doi.org/10.3390/galaxies5010012