Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback

SR Ward, CM Harrison, T Costa… - Monthly Notices of the …, 2022 - academic.oup.com
Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the
quenching of massive galaxies in the vast majority of modern galaxy evolution models …

The star-forming main sequence of the host galaxies of low-redshift quasars

MY Zhuang, LC Ho - The Astrophysical Journal, 2022 - iopscience.iop.org
We investigate the star-forming main sequence of the host galaxies of a large, well-defined
sample of 453 redshift∼ 0.3 quasars with previously available star formation rates by …

Stellar and black hole assembly in z < 0.3 infrared-luminous mergers: intermittent starbursts versus super-Eddington accretion

D Farrah, A Efstathiou, J Afonso… - Monthly Notices of …, 2022 - academic.oup.com
We study stellar and black hole mass assembly in a sample of 42 infrared-luminous galaxy
mergers at z< 0.3 by combining results from radiative transfer modelling with archival …

[HTML][HTML] The Close AGN Reference Survey (CARS)-IFU survey data and the BH mass dependence of long-term AGN variability

B Husemann, M Singha, J Scharwächter… - Astronomy & …, 2022 - aanda.org
Context. Active galactic nuclei (AGN) are thought to be intimately connected with their host
galaxies through feeding and feedback processes. A strong coupling is predicted and …

A radio-jet-driven outflow in the Seyfert 2 galaxy NGC 2110?

LP de Arriba, A Alonso-Herrero… - Astronomy & …, 2023 - aanda.org
We present a spatially resolved study of the ionized gas in the central 2 kpc of the Seyfert 2
galaxy NGC 2110 and investigate the role of its moderate-luminosity radio jet (kinetic radio …

The M•–σe relation for local type 1 AGNs and quasars

J Molina, LC Ho, KK Knudsen - Astronomy & Astrophysics, 2024 - aanda.org
We analyzed Multi Unit Spectroscopic Explorer observations of 42 local z≲ 0.1 type 1 active
galactic nucleus (AGN) host galaxies taken from the Palomar-Green quasar sample and the …

The collisional and photoionized plasma in the polarized NLS1 galaxy Mrk 1239

MZ Buhariwalla, LC Gallo, J Mao… - Monthly Notices of …, 2023 - academic.oup.com
Mrk 1239 is a highly polarized NLS1 in the optical band, whose 0.3–3 keV spectrum has
remained remarkably consistent over more than two decades of observation. Previous …

Exploring the connection between AGN radiative feedback and massive black hole spin

F Bollati, A Lupi, M Dotti, F Haardt - Astronomy & Astrophysics, 2024 - aanda.org
We present a novel implementation for active galactic nucleus (AGN) feedback through
ultrafast winds in the code GIZMO. Our feedback recipe accounts for the angular …

The Close AGN Reference Survey (CARS)-Tracing the circumnuclear star formation in the super-Eddington NLS1 Mrk 1044

N Winkel, B Husemann, TA Davis… - Astronomy & …, 2022 - aanda.org
Context. The host galaxy conditions for rapid supermassive black hole growth are poorly
understood. Narrow-line Seyfert 1 (NLS1) galaxies often exhibit high accretion rates and are …

Unraveling the Complex Structure of AGN-driven Outflows. VI. Strong Ionized Outflows in Type 1 AGNs and the Outflow Size–Luminosity Relation

C Kim, JH Woo, R Luo, A Chung, J Baek… - The Astrophysical …, 2023 - iopscience.iop.org
We present spatially resolved gas kinematics, ionization, and energetics of 11 type 1 and 5
type 2 active galactic nuclei (AGNs) with strong ionized gas outflows at z< 0.3 using Gemini …