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 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.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-11-11
DOI
https://doi.org/10.3847/2041-8213/ae157d
Primary Topic
Astrophysical Phenomena and Observations
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article
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article

Detection of Compton Scattering in the Jet of 3C 84

Fabian Kislat, Laura Di Gesu, Thibault Barnouin, Dawoon E. Kim et al.
The Astrophysical Journal Letters
Astrophysical Phenomena and Observations
article

Detection of Compton Scattering in the Jet of 3C 84

Fabian Kislat, Laura Di Gesu, Thibault Barnouin, Dawoon E. Kim, A. A. Vasilyev, Daniel Morcuende, Chien‐Ting Chen, A. Sota, A. Kraus, Ioannis Liodakis, А. В. Жовтан, Pouya M. Kouch, Y. Y. Kovalev, E. Costa, Garrett K. Keating, F. Tavecchio, E. Angelakis, Diego Álvarez-Ortega, Sincheol Kang, M. Lynne Saade, P. Soffitta, A. Strigachev, Jorge Otero-Santos, Martin C. Weisskopf, Е. Г. Ларионова, Yu. V. Troitskaya, С. С. Савченко, V. Fallah Ramazanı, Myung-Jin Nam, O. J. Roberts, I. Myserlis, T. S. Grishina, I. Agudo, Francesco Tombesi, Ramprasad Rao, Frédéric Marin, D. A. Morozova, Steven R. Ehlert, Sudip Chakraborty, Stephen L. O’Dell, Hyeon‐Woo Jeong, F. J. Aceituno, E. N. Kopatskaya, I. S. Troitskiy, Riccardo Ferrazzoli, Sang-Sung Lee, G. Bonnoli, Giorgio Galanti, E. Lindfors, V. Casanova, K. Nilsson, Г. А. Борман, Douglas A. Swartz, Chanwoo Song, Whee Yeon Cheong, Georgios Filippos Paraschos, C. Casadio, Jenni Jormanainen, R. Middei, E. Churazov, Mark Gurwell, L. Pacciani, Alan P. Marscher, P. Kaaret, Ajay Ratheesh, Anna Trindade Falcão, R. Bachev, M. Roncadelli, V. Piirola, Shan Li, Sang-Hyun Kim, V. A. Hagen-Thorn, Juan Escudero, Tapio Pursimo, Jacob Casey, Gabriel Emery, S. G. Jorstad, Ekaterina V. Shishkina, Ildar Khabibulin
article en

Abstract

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.

The Astrophysical Journal LettersVol. 994(1)
Openalex Percentile: Top 77%
Astrophysical Phenomena and Observations
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