Extraordinary Activity in the BL Lac Object OJ~287
Abstract
We use a continuous wavelet transform to analyze more than two decades of data for the BL~Lac object OJ~287 acquired as part of the UMRAO variability program. We find clear evidence for a persistent modulation of the total flux and polarization with period years, and for another signal that dominates activity in the 1980s with period years. The relationship between these two variations can be understood in terms of a `shock-in-jet' model, in which the longer time scale periodicity is associated with an otherwise quiescent jet, and the shorter time scale activity is associated with the passage of a shock; the different periodicities of these two components may reflect different internal conditions of the two flow domains, leading to different wave speeds, or different contractions of a single underlying periodicity, due to the different Doppler factors of the two flow components. We suggest that the modulation arises from a wave driven by some asymmetric disturbance close to the central engine. The periodic behavior in polarization exhibits excursions in which correspond to a direction from the VLBI jet axis. This behavior is not explained by the random walk in the - plane which is expected from models in which a pattern of randomly aligned magnetic field elements propagate across the visible portion of the flow, and suggests a small amplitude, cyclic variation in the flow direction in that part of the flow that dominates cm-wavelength emission.
Cite
@article{arxiv.astro-ph/9802275,
title = {Extraordinary Activity in the BL Lac Object OJ~287},
author = {Philip A. Hughes and Hugh D. Aller and Margo F. Aller},
journal= {arXiv preprint arXiv:astro-ph/9802275},
year = {2009}
}
Comments
Text: 22 pages, PostScript line figures: 10 pages, GIF color figures: 7. High quality PostScript versions of the GIF images may be obtained from the "Wavelets/First Results" section of http://www.astro.lsa.umich.edu/users/hughes/, or by anon. ftp from file get/hughes/waves.tar.gz at ra.astro.lsa.umich.edu. Submitted to Ap. J