activity
20122026
most citedGalactic winds driven by cosmic-ray streaming

235 citations · 520 across the 52 of their papers we have counts for

collaborators
Showing 2024 · astro-ph.GAShow all

11 papers · 2 filters

astro-ph.GA2024★ 7 cited

Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts

Larissa Tevlin, Thomas Berlok, Christoph Pfrommer +6

Observations of Faraday rotation and synchrotron emission in galaxy clusters imply large-scale magnetic fields with strengths possibly extending back to . Non-ra…

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…

astro-ph.GA2024★ 4 cited

Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (II) The inside-out growth of discs

Federico G. Iza, Sebastián E. Nuza, Cecilia Scannapieco +6

We investigate the growth of stellar discs in Milky Way-mass galaxies using the magnetohydrodynamical simulations of the Auriga Project in a full cosmological context. We focus on…

astro-ph.GA2024

The effect of local photoionization on the galaxy properties and the circumgalactic medium in simulations of Milky Way-sized galaxies

Bocheng Zhu, Volker Springel

In this study, we investigate the impact of local stellar radiation in cosmological zoom simulations of the formation of Milky Way-sized galaxies. We include the radiation field as…

astro-ph.GA2024★ 4 cited

The influence of baryons on low-mass haloes

Haonan Zheng, Sownak Bose, Carlos S. Frenk +6

The Voids-within-Voids-within-Voids (VVV) project used dark-matter-only simulations to study the abundance and structure of dark matter haloes over the full mass range populated in…

astro-ph.GA2024★ 6 cited

Brightest Cluster Galaxy Offsets in Cold Dark Matter

Cian Roche, Michael McDonald, Josh Borrow +7

The distribution of offsets between the brightest cluster galaxies of galaxy clusters and the centroid of their dark matter distributions is a promising probe of the underlying dar…

astro-ph.GA2024

The evolutionary path of void galaxies in TNG300 simulation

Agustín Rodríguez-Medrano, Volker Springel, Federico Stasyszyn +1

The properties of galaxies in low-density regions of the universe suggest an interplay between galaxy formation and environment. However, the specific reason why this particular la…