2004/10/07 by Frank M. Rieger · 1 citation
Physics and Astronomy · #astro-ph
paper · pdf · doi:10.1086/426018
published as Astrophys.J. 615 (2004) L5-L8 · 10 pages, ApJ Letters in press
arxiv created 2004/10/07 · arxiv updated 2009/12/01
Periodicities in blazar light curves may be related to helical trajectories in extragalactic radio jets by differential Doppler boosting effects. We consider ballistic and non-ballistic (i.e., radial) trajectories and discuss three possible periodic driving mechanisms for the origin of helical jet paths, namely, orbital motion in a binary black hole system (BBHS), jet precession, and intrinsic jet rotation. It is shown that precessional-driven ballistic motion is unlikely to result in observable periods of less than several tens of years. We demonstrate that for non-ballistic helical motion the observed period is generally strongly shortened relative to the real physical driving period because of light-travel time effects. Internal jet rotation may thus account for observed periods P\rm obs ≤ 10 days. Periodicity due to orbital-driven (non-ballistic) helical motion, on the other hand, is usually constrained to periods of P\rm obs ≥ 10 days, while Newtonian-driven precession is unlikely to be responsible for periodicity on a timescale P\rm obs ≤ 100 days but may well be associated with periods of P\rm obs ≥ 1 yr.