Work

Detection of Compton Scattering in the Jet of 3C 84

Year: 2025
Type: article
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 γ -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 Ms coinciding with a flare in γ -rays. This is the longest observation for a radio-loud active galaxy, which allowed us to reach unprecedented sensitivity, leading to the detection of an X-ray polarization degree of Π X = 4.2% ± 1.3% (∼3.2 σ confidence) at an X-ray electric vector polarization angle of ψ X = 163° ± 9°, which 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 place downstream, away from the supermassive black hole.
Institutions: FORTH Institute of Astrophysics, Max Planck Institute for Radio Astronomy, Foundation for Research and Technology Hellas, Marshall Space Flight Center, Centre National de la Recherche Scientifique, Observatoire astronomique de Strasbourg, Université de Strasbourg, University of Turku, Aarhus University, Nordic Optical Telescope, Astronomical Observatory of Rome, Agenzia Spaziale Italiana, Center for Astrophysics Harvard & Smithsonian, National Institute for Astrophysics, Goddard Space Flight Center, Boston University, St Petersburg University, Instituto de Astrofísica de Andalucía, University of New Hampshire, Institute for Space Astrophysics and Planetology, Physical Research Laboratory, Universities Space Research Association, University of Rome Tor Vergata, Istituto Nazionale di Fisica Nucleare, Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata, Brera Astronomical Observatory, Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Bulgarian Academy of Sciences, Institute of Astronomy and National Astronomical Observatory, Crimean Astrophysical Observatory, Pulkovo Observatory, Instituto de Radioastronomía Milimétrica, Korea Astronomy and Space Science Institute, Korea University of Science and Technology, University of Crete, National and Kapodistrian University of Athens, Aalto University, Max Planck Institute for Astrophysics, Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano, Ludwig-Maximilians-Universität München, Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, University of Chicago
Language: English
Open Access status: gold
Estimated APC paid: $2,400
OpenAlex ID: W4415949725
FWCI: 1.417
Cites: 100
Cited by: 3
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