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20212026
most citedSmall-scale dynamos: From idealized models to solar and stellar applications

36 citations · 150 across the 18 of their papers we have counts for

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8 papers · 1 filter

astro-ph.GA2026

X-ray Characterization of Galaxy Groups and Hickson Groups in COSMOS-Web to z~3.8 I. X-ray Luminosity Function Evolution

Ghassem Gozaliasl, Günther Hasinger, Gavin Leroy +35

Galaxy groups are the dominant halo environment in the Universe and a sensitive laboratory for feedback and gas-cycling physics, yet a uniform, intermediate-redshift X-ray characte…

astro-ph.GA2025

Asymptotic behaviour of galactic small-scale dynamos at modest magnetic Prandtl number

Frederick A. Gent, Mordecai-Mark Mac Low, Maarit J. Korpi-Lagg +2

Magnetic fields are critical at many scales to galactic dynamics and structure, including multiphase pressure balance, dust processing, and star formation. Dynamo action determines…

astro-ph.GA2025★ 5 cited

COSMOS Web: Morphological quenching and size-mass evolution of brightest group galaxies from z = 3.7

Ghassem Gozaliasl, Lilan Yang, Jeyhan Kartaltepe +47

We present a comprehensive study of the structural evolution of Brightest Group Galaxies (BGGs) from redshift to using the \textit{James Webb Space Telesc…

astro-ph.GA2025

COSMOS-Web: Estimating Physical Parameters of Galaxies Using Self-Organizing Maps

Fatemeh Abedini, Ghassem Gozaliasl, Akram Hasani Zonoozi +38

The COSMOS-Web survey, with its unparalleled combination of multiband data, notably, near-infrared imaging from JWST's NIRCam (F115W, F150W, F277W, and F444W), provides a transform…

astro-ph.GA2025★ 12 cited

The COSMOS-Web deep galaxy group catalog up to

Greta Toni, Ghassem Gozaliasl, Matteo Maturi +41

Galaxy groups with and up to a few tens of members are the most common galaxy environment, marking the transition between field and massive clu…

astro-ph.GA2024★ 1 cited

Computational approaches to modeling dynamos in galaxies

Maarit J. Korpi-Lagg, Mordecai-Mark Mac Low, Frederick A. Gent

Galaxies are observed to host magnetic fields with a typical total strength of around 15microgauss. A coherent large-scale field constitutes up to a few microgauss of the total, wh…

astro-ph.GA2023★ 18 cited

Transition from small-scale to large-scale dynamo in a supernova-driven, multiphase medium

Frederick A. Gent, Mordecai-Mark Mac Low, Maarit J. Korpi-Lagg

Magnetic fields are widely recognised as critical at many scales to galactic dynamics and structure, including multiphase pressure balance, dust processing, and star formation. Usi…

astro-ph.GA2022★ 27 cited

The small-scale dynamo in a multiphase supernova-driven medium

Frederick A. Gent, Mordecai-Mark Mac Low, Maarit J. Korpi-Lagg +1

Magnetic fields grow quickly, even at early cosmological times, suggesting the action of a small-scale dynamo (SSD) in the interstellar medium (ISM) of galaxies. Many studies have…