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From the 1 of 6 linked papers with an AI index.

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6 papers

astro-ph.GA2026

Too many quiescent late-type galaxies or a matter of misclassification?

J. L. Tous, S. I. Raimundo, H. Domínguez Sánchez

In the local Universe, the terms late-type and early-type are used to describe, respectively, disc galaxies with spiral arms and more bulge-dominated systems lacking spiral structu…

astro-ph.GA2026

Fuelling the central region of galaxies with misaligned gas accretion

J. L. Tous, S. I. Raimundo, R. Riffel +3

The paper investigates how gas that is kinematically misaligned with a galaxy’s disk fuels central star formation and potentially black‑hole growth, finding that this accretion sus…

astro-ph.GA2025

Stellar-gas kinematic misalignments in EAGLE: enhanced SMBH growth in misaligned galaxies

Maximilian K. Baker, Timothy A. Davis, Freeke van de Voort +1

Stellar-gas kinematic misalignments are a transient phenomenon observed in of the local galaxy population. According to current models, misaligned gas is expected to los…

astro-ph.GA2025

A Stellar Dynamical Mass for the Central Black Hole in MCG06-30-15

Nabanita Das, Misty C. Bentz, Eugene Vasiliev +4

We present the stellar dynamical mass of the central black hole in the nearby Seyfert galaxy MCG06-30-15 using the Schwarzschild orbit-superposition method implemented in the op…

astro-ph.GA2025

Kinematic misalignment as a driver of black hole activity in galaxies with external interactions

Sandra I. Raimundo, Rogerio Riffel, Song-lin Li +6

The process of Active Galactic Nuclei (AGN) fuelling relies on the transport of gas across several orders of magnitude in physical scale until the gas reaches the supermassive blac…

astro-ph.GA2025

Flares in the Changing Look AGN Mrk 590. II: Deep X-ray observations reveal a Comptonizing inner accretion flow

Daniel Lawther, Marianne Vestergaard, Sandra Raimundo +2

Mrk 590 is a Changing Look AGN currently in an unusual repeat X-ray and UV flaring state. Here, we report on deep X-ray observations with XMM-Newton, NuSTAR, and NICER, obtained at…