Active galactic nuclei (AGN) are powered by the accretion of material onto a supermassive
black hole (SMBH) and are among the most luminous objects in the Universe. However, the …

This review describes recent developments related to the unified model of active galactic
nuclei (AGNs). It focuses on new ideas about the origin and properties of the central …

Polycyclic aromatic hydrocarbon (PAH) molecules are abundant and widespread throughout
the Universe, as revealed by their distinctive set of emission bands at 3.3, 6.2, 7.7, 8.6, 11.3 …

Aims. We investigate the fueling and the feedback of star formation and nuclear activity in
NGC 1068, a nearby (D= 14 Mpc) Seyfert 2 barred galaxy, by analyzing the distribution and …

The advent of high-angular-resolution IR and submillimeter interferometry allows for
spatially resolved observations of the parsec-scale environment of active galactic nuclei …

We investigate the effect of active galactic nucleus (AGN) variability on the observed
connection between star formation and black hole accretion in extragalactic surveys. Recent …

Molecular gas serves as a key probe of the complex interplay between black hole accretion
and star formation in the host galaxies of active galactic nuclei (AGNs). We use CO (2–1) …

We present cosmological hydrodynamic simulations of a quasar-mass halo (M halo≈ 10
12.5 M⊙ at z= 2) that for the first time resolve gas transport down to the inner 0.1 pc …

Polycyclic aromatic hydrocarbons (PAHs) are carbon-based molecules that are ubiquitous in
a variety of astrophysical objects and environments. In this work we use JWST/MIRI MRS …

We present an analysis of [] Oi 63,[Oiii] 88,[Nii] 122, and [] Cii 158 far-infrared (FIR) fine-
structure line observations obtained with Herschel/PACS, for∼ 240 local luminous infrared …