A multiband study and exploration of the radio wave - $\gamma$-ray connection in 3C 84
G. F. Paraschos, V. Mpisketzis, J.-Y. Kim, G. Witzel, T. P. Krichbaum,, J. A. Zensus, M. A. Gurwell, A. L\"ahteenm\"aki, M. Tornikoski, S. Kiehlmann,, A. C. S. Readhead

TL;DR
This study analyzes decades of radio and gamma-ray data from 3C 84, revealing jet properties, magnetic field estimates, and the connection between radio and gamma-ray flares, supporting the Blandford-Znajek jet launching mechanism.
Contribution
It provides a detailed multiband analysis of 3C 84, including jet location, magnetic field strength, and flare timing, using cross-correlation and Gaussian process regression, which advances understanding of jet physics.
Findings
Jet particle and magnetic energy are in equipartition.
The jet apex is located 22-645 R_s upstream of the radio core.
Gamma-ray flares are associated with radio flare ejections.
Abstract
Total intensity variability light curves offer a unique insight into the ongoing debate about the launching mechanism of jets. For this work, we utilise the availability of radio and -ray light curves over a few decades of the radio source 3C 84 (NGC 1275). We calculate the multiband time lags between the flares identified in the light curves via discrete cross-correlation and Gaussian process regression. We find that the jet particle and magnetic field energy densities are in equipartition (). The jet apex is located ( pc) upstream of the 3 mm radio core; at that position, the magnetic field amplitude is G. Our results are in good agreement with earlier studies, which utilised very-long-baseline interferometry. Furthermore, we investigate…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Solar and Space Plasma Dynamics · Magnetic confinement fusion research
