A multiband study and exploration of the radio wave - -ray connection in 3C 84
arXiv:2210.09795 · doi:10.1051/0004-6361/202244814
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 the temporal relation between the ejection of radio and -ray flares. Our results are in favour of the -ray emission being associated with the radio emission. We are able to tentatively connect the ejection of features identified at 43 and 86 GHz to prominent -ray flares. Finally, we compute the multiplicity parameter and the Michel magnetisation and find that they are consistent with a jet launched by the Blandford & Znajek 1977 mechanism.
arXiv comment13 pages, 6 figures, accepted for publication in A&A
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