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Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback
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Ultrafast Outflows: Galaxy-Scale Active Galactic Nucleus Feedback
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A Study on Active Galactic Nucleus Variability
2022Active Galactic Nuclei (AGNs) are accreting supermassive black holes at the center of galaxies, known for rich spectral features and multi-time scale variability in their electromagnetic emission. The origin of the variability in AGN light curves can be either intrinsic, meaning related processes that take place inside the AGN system, or extrinsic, i.e.
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IC4553: Masers Around an Active Galactic Nucleus
Publications of the Astronomical Society of Australia, 1984AbstractThe galaxy IC4553 (Arp 220) is a peculiar galaxy having a redshift of 0.02. It has been variously described as consisting of a symbiotic pair of galaxies, as having a highly peculiar pair of nuclei, or as consisting of a nucleus bisected by a dust lane. In addition, it exhibits OH maser emission which is both the most intrinsically luminous (by
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ACTIVE GALACTIC NUCLEUS FEEDBACK IN GIANTS AND DWARFS
2022Feedback from Active Galactic Nucleus (AGN) may play a critical role in the coevolution of galaxies and supermassive black holes (SMBH). Specifically, AGN feedback may quench star formation, suppress baryon-to-dark matter mass ratio, shape galaxy morphology, impact the circumgalactic (CGM)/intergalactic medium (IGM), and regulate SMBH accretion. One of
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Multiple shock acceleration in active galactic nucleus jets
Proceedings of 7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy — PoS(Gamma2022), 2023Ana Laura Müller, Anabella Araudo
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An energetic hot wind from the low-luminosity active galactic nucleus M81*
Nature Astronomy, 2021Fangzheng Shi, Zhiyuan Li, Feng Yuan
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Radiation drag in relativistic active galactic nucleus jets
Monthly Notices of the Royal Astronomical Society, 1996M. Sikora +3 more
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