activity
20162026
most citedResolving small-scale cold circumgalactic gas in TNG50

189 citations · 1.9k across the 85 of their papers we have counts for

collaborators
Showing 2024 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA2024★ 1 cited

A grand-design spiral galaxy with an ordered magnetic field at redshift 2.6 as resolved with ALMA and gravitational lensing

W. de Roo, S. Vegetti, D. M. Powell +3

Magnetic fields play an important role in the evolution of galaxies and in shaping the dynamics of their inter-stellar medium. However, the formation history of magnetic fields fro…

astro-ph.GA2024★ 1 cited

Anisotropic thermal conduction on a moving mesh for cosmological simulations

Rosie Y. Talbot, Rüdiger Pakmor, Christoph Pfrommer +4

In weakly collisional, strongly magnetised plasmas such as the intracluster medium (ICM), hot accretion flows and the solar corona, the transport of heat and momentum occurs primar…

astro-ph.GA2024

Moving-mesh non-ideal magnetohydrodynamical simulations of the collapse of cloud cores to protostars

Alexander C. Mayer, Oliver Zier, Thorsten Naab +5

Magnetic fields have been shown both observationally and through theoretical work to be an important factor in the formation of protostars and their accretion disks. Accurate model…

astro-ph.GA2024★ 2 cited

Environment matters: stronger magnetic fields in satellite galaxies

Maria Werhahn, Rüdiger Pakmor, Rebekka Bieri +3

Magnetic fields are ubiquitous in the universe and an important component of the interstellar medium. It is crucial to accurately model and understand their properties in different…

astro-ph.GA2024★ 10 cited

Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models

Eric Zhang, Laura V. Sales, Federico Marinacci +6

Simulations of galaxy formation are mostly unable to resolve the energy-conserving phase of individual supernova events, having to resort to subgrid models to distribute the energy…

astro-ph.GA2024★ 8 cited

Bar formation and evolution in the cosmological context: Inputs from the Auriga simulations

Francesca Fragkoudi, Robert Grand, Rüdiger Pakmor +3

Galactic bars drive the internal evolution of spiral galaxies, while their formation is tightly coupled to the properties of their host galaxy and dark matter halo. To explore what…