Detection of Compton scattering in the jet of 3C 84

Abstract

3C 84 is the brightest cluster galaxy in the Perseus Cluster. It is among the closest radio-loud active galaxies and among the very few that can be detected from low frequency radio up to TeV $\gamma$-rays. Here we report on the first X-ray polarization observation of 3C~84 with the Imaging X-ray Polarimetry Explorer, for a total of 2.2 Msec that coincides with a flare in $\gamma$-rays. This is the longest observation for a radio-loud active galaxy that allowed us to reach unprecedented sensitivity, leading to the detection of an X-ray polarization degree of ${\mathrm{\Pi }}_{\mathrm{X}}=4.2\pm 1.3\%$ ($\sim 3.2\sigma$ confidence) at an X-ray electric vector polarization angle of ${\psi }_{\mathrm{X}}=163^{\circ }\pm 9^{\circ }$, that is aligned with the radio jet direction on the sky. Optical polarization observations show fast variability about the jet axis as well. Our results strongly favor models in which X-rays are produced by Compton scattering from relativistic electrons -- specifically Synchrotron Self-Compton -- that takes places downstream, away from the supermassive black hole.

arXiv comment21 pages, 13 figure, 1 Table, published in APJL

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