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Theory of winds in AGNs

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

I present a brief review of theory of winds in active galactic nuclei (AGN). Magnetic, radiation, and thermal driving likely operate in AGN. In many cases, it is difficult to distinguish, both from observational and theoretical point of view, which of these wind driving mechanisms dominates in producing winds. Therefore, I focus on specific theoretical predictions which could help to improve our understanding of the physics of AGN winds.

fields

astro-ph.GA 2

years

2026 2

representative citing papers

Unification models of Active Galactic Nuclei

astro-ph.GA · 2026-06-10 · conditional · novelty 2.0

A review of AGN unification concluding that whether a black-hole-powered nucleus appears obscured depends on inclination, Eddington ratio (radiative feedback), and host-galaxy merger/redshift evolution.

citing papers explorer

Showing 2 of 2 citing papers.

  • Flagging Super-Eddington Candidates among Jetted, {\gamma}-Ray-Emitting AGN astro-ph.GA · 2026-06-09 · unverdicted · none · ref 29 · internal anchor

    The E1/MS framework flags super-Eddington candidates in jetted gamma-ray AGN, with some showing jet-consistent radio properties and gamma-ray NLS1s showing xA spectra.

  • Unification models of Active Galactic Nuclei astro-ph.GA · 2026-06-10 · conditional · none · ref 164 · internal anchor

    A review of AGN unification concluding that whether a black-hole-powered nucleus appears obscured depends on inclination, Eddington ratio (radiative feedback), and host-galaxy merger/redshift evolution.