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.
13 pages, 6 figures, accepted for publication in A&A
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- Observational Evidence to Support a Dense Ambient Medium Shaping the Jet in 3C 84
- Revisiting the proton synchrotron radiation in blazar jets: Possible contributions from X-ray to -ray bands
- Closing the feedback-feeding loop of the radio galaxy 3C 84
- The dynamics of the parsec-scale jet in the neutrino blazar PKS 0735+178
- Relationship between the ray variability and the pc-scale jet in the blazar 3C 454.3
- Where within the 3C 84 jet are -rays produced?
- Detection of Compton scattering in the jet of 3C 84
- Millimeter VLBI constraints on the central magnetic field and symmetric jet production in the twin-jet galaxy NGC 1052