{ "id": "2003.01911", "version": "v1", "published": "2020-03-04T06:34:06.000Z", "updated": "2020-03-04T06:34:06.000Z", "title": "Quasi-periodic Oscillation and Evidence of a Curved Jet in the Blazar 3C 454.3", "authors": [ "Arkadipta Sarkar", "Alok C. Gupta", "Varsha R. Chitnis", "Paul J. Wiita" ], "comment": "10 pages, 5 figures; Submitted to ApJL", "categories": [ "astro-ph.HE" ], "abstract": "We report the detection of a quasi-periodic oscillation (QPO) in light curves of the blazar 3C 454.3. Periodic flux modulation was detected simultaneously in both $\\gamma$--ray and optical wavebands with a dominant period of $\\sim 47$ days. This period has a significance of over $4.2\\sigma$ in the \\textit{Fermi} $\\gamma$--ray waveband and around $2.4\\sigma$ in the optical V band. This QPO lasted for over 450 days (from MJD 56800 to 57250) resulting in over nine observed periods which is among the highest number of periods ever detected in a blazar light curve. The lower significance of the dominant period in optical wavebands is attributed to the absence of optical data for a number of QPO cycles due to the daytime transit of the source. We explore several physical models to explain the origin of this transient quasi-periodic modulation in the observed flux with a month-like period. These scenarios include a binary black hole system, a hotspot orbiting close to the innermost stable circular orbit of the supermassive black hole, and precessing jets. We conclude that the most likely scenario involves a region of enhanced emission moving helically inside a jet. Also, a curvature of $\\sim 0.05^{\\circ}$ pc$^{-1}$ in the jet fits the emission much better than does a straight blazar jet.", "revisions": [ { "version": "v1", "updated": "2020-03-04T06:34:06.000Z" } ], "analyses": { "keywords": [ "blazar 3c", "quasi-periodic oscillation", "curved jet", "emission moving helically inside", "dominant period" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }