A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviour
C.M. Raiteri, M. Villata, M.I. Carnerero, S.O. Kurtanidze, D.O., Mirzaqulov, E. Ben\'itez, G. Bonnoli, D. Carosati, J.A. Acosta-Pulido, I., Agudo, T.S. Andreeva, G. Apolonio, R. Bachev, G.A. Borman, V. Bozhilov, L.F., Brown, W. Carbonell, C. Casadio, W.P. Chen, G. Damljanovic

TL;DR
This study models blazar variability using a twisting, wiggling jet structure, linking optical, radio, and gamma-ray emissions to a dynamic geometric scenario involving plasma filaments in a double-helix configuration.
Contribution
It introduces a geometric twisting jet model to explain multi-wavelength variability in blazars, supported by multi-year observational data of BL Lacertae.
Findings
Optical-radio correlation with a 120-day lag supports a common jet origin.
Gamma-ray emission is co-spatial with optical emission, consistent with SSC models.
Wiggling jet motion explains long-term multi-wavelength variability.
Abstract
Blazars are beamed active galactic nuclei known for their strong multi-wavelength variability on timescales from years down to minutes. We aim to investigate the suitability of the twisting jet model presented in previous works to explain the multi-wavelength behaviour of BL Lacertae, the prototype of one of the blazar classes. According to this model, the jet is inhomogeneous, curved, and twisting, and the long-term variability is due to changes in the Doppler factor due to variations in the orientation of the jet-emitting regions. We analysed optical data of the source obtained during monitoring campaigns organised by the Whole Earth Blazar Telescope (WEBT) in 2019-2022, together with radio data from the WEBT and other teams, and gamma-ray data from the Fermi satellite. In this period, BL Lacertae underwent an extraordinary activity phase, reaching its historical optical and gamma-ray…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gyrotron and Vacuum Electronics Research
