Ultra-thick warm absorbers form a new subclass of AGN ionized outflows with exceptionally high column densities and moderate ionization that drive strong variability and may connect to ultra-fast outflows.
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2 Pith papers cite this work. Polarity classification is still indexing.
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HE 1237-2252 exhibits a changing-look event driven by intrinsic accretion-rate variations, revealing a two-component broad-line region consisting of virialized gas at ~27 light-days and disk emission at larger radii.
citing papers explorer
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Ultra-thick warm absorbers: Enlarging the parameter space of AGN ionised outflows
Ultra-thick warm absorbers form a new subclass of AGN ionized outflows with exceptionally high column densities and moderate ionization that drive strong variability and may connect to ultra-fast outflows.
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A Changing-Look Seyfert Discovered by eROSITA Reveals a Two-Component Broad-Line Region
HE 1237-2252 exhibits a changing-look event driven by intrinsic accretion-rate variations, revealing a two-component broad-line region consisting of virialized gas at ~27 light-days and disk emission at larger radii.