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Radio galaxies and feedback from AGN jets

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arxiv 2003.06137 v1 pith:C7XBORVJ submitted 2020-03-13 astro-ph.HE astro-ph.GA

M. J. Hardcastle , J. H. Croston This is my paper · ORCID
classification astro-ph.HEastro-ph.GA
keywords galaxiesradiofeedbackdiscussgalaxylarge-scaleunderstandingaccretion
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We review current understanding of the population of radio galaxies and radio-loud quasars from an observational perspective, focusing on their large-scale structures and dynamics. We discuss the physical conditions in radio galaxies, their fuelling and accretion modes, host galaxies and large-scale environments, and the role(s) they play as engines of feedback in the process of galaxy evolution. Finally we briefly summarise other astrophysical uses of radio galaxy populations, including the study of cosmic magnetism and cosmological applications, and discuss future prospects for advancing our understanding of the physics and feedback behaviour of radio galaxies.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Time-Dependent Cosmic Ray Halos from Bursty Star Formation and Active Galactic Nuclei: Semi-Analytic Formalism and Galaxy Formation Implications

    astro-ph.GA 2025-09 conditional novelty 6.0 of 10

    Time-dependent injection from bursty star formation or episodic black hole accretion substantially modifies cosmic ray pressure profiles in massive galaxy halos, flattening them at large radii relative to steady-state...

  2. CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    CRESCENDO's spectral cosmic-ray solver now includes improved energy-loss processes, non-ultra-relativistic energy/pressure integrals, and supernova-remnant template injection.

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