activity
20162026
most citedGas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution

111 citations · 363 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2026

The diverse nature of spiral arms in the Auriga Superstars cosmological hydrodynamic simulations

Robert J J Grand, Francesca Fragkoudi, Rüdiger Pakmor +4

The dynamical nature and formation mechanism(s) of galactic spiral arms remain long-standing problems in astrophysics. Most theoretical work is based on analytic calculations or id…

astro-ph.GA2025

Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal): IV. On the inner Milky Way stellar age distribution

Tomás Ruiz-Lara, David Mirabal, Carme Gallart +15

The Milky Way's inner region is dominated by a stellar bar and a boxy-peanut shaped bulge. However, which stellar populations inhabit the inner Galaxy or how star formation proceed…

astro-ph.GA2025

Unveiling the Impact of Cosmic Rays on the Disc Sizes and Outflows from Dwarf Scales to Galaxy Groups

Rebekka Bieri, Rüdiger Pakmor, Freeke van de Voort +4

Cosmic rays (CRs) are a non-thermal energy component in the interstellar and circumgalactic medium (CGM) that can act as an additional feedback channel beyond thermal and kinetic f…

astro-ph.GA2025★ 2 cited

Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations

Ruediger Pakmor, Francesca Fragkoudi, Robert J. J. Grand +7

Cosmological hydrodynamical simulations have become an indispensable tool to understand galaxies. However, computational constraints still severely limit their numerical resolution…

astro-ph.GA2025★ 7 cited

Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model

Ruediger Pakmor, Rebekka Bieri, Francesca Fragkoudi +6

Numerical simulations have become an indispensable tool in astrophysics. To interpret their results, it is critical to understand their intrinsic variability, that is, how much the…

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

Understanding gas mixing in the circumgalactic medium

Hilay Shah, Freeke van de Voort, Amit Seta +1

We study gas mixing in a simulated Milky Way-mass galaxy's circumgalactic medium (CGM) using cosmological `zoom-in' simulations. We insert tracer dyes in the CGM with different gas…

astro-ph.GA2024★ 2 cited

The halo mass dependence of physical and observable properties in the circumgalactic medium

Andrew W. S. Cook, Freeke van de Voort, Rüdiger Pakmor +1

We study the dependence of the physical and observable properties of the CGM on its halo mass. We analyse 22 simulations from the Auriga suite of high resolution cosmological `zoom…

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.GA2022★ 9 cited

Formation and fate of low metallicity stars in IllustrisTNG50

Ruediger Pakmor, Christine M. Simpson, Freeke van de Voort +6

Low metallicity stars give rise to unique spectacular transients and are of immense interest for understanding stellar evolution. Their importance has only grown further with the r…

astro-ph.GA2019★ 111 cited

Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution

Robert J. J. Grand, Freeke van de Voort, Jolanta Zjupa +7

Using a set of 15 high-resolution magnetohydrodynamic cosmological simulations of Milky Way formation, we investigate the origin of the baryonic material found in stars at redshift…

astro-ph.GA2019★ 83 cited

Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies

Freeke van de Voort, Rüdiger Pakmor, Robert J. J. Grand +3

We use cosmological, magnetohydrodynamical simulations of Milky Way-mass galaxies from the Auriga project to study their enrichment with rapid neutron capture (r-process) elements.…

astro-ph.GA2018★ 39 cited

The impact of feedback and the hot halo on the rates of gas accretion onto galaxies

Camila A. Correa, Joop Schaye, Freeke van de Voort +2

We investigate the physics that drives the gas accretion rates onto galaxies at the centers of dark matter haloes using the EAGLE suite of hydrodynamical cosmological simulations.…

astro-ph.GA2018★ 36 cited

An ALMA view of star formation efficiency suppression in early-type galaxies after gas-rich minor mergers

Freeke van de Voort, Timothy A. Davis, Satoki Matsushita +6

Gas-rich minor mergers contribute significantly to the gas reservoir of early-type galaxies (ETGs) at low redshift, yet the star formation efficiency (SFE; the star formation rate…

astro-ph.GA2017★ 15 cited

On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium

Freeke van de Voort, Eliot Quataert, Claude-André Faucher-Giguère +5

We quantify the gas-phase abundance of deuterium and fractional contribution of stellar mass loss to the gas in cosmological zoom-in simulations from the Feedback In Realistic Envi…

astro-ph.GA2016★ 57 cited

The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev-Zel'dovich effect and soft X-ray emission

Freeke van de Voort, Eliot Quataert, Philip F. Hopkins +5

The thermal Sunyaev-Zel'dovich (SZ) effect and soft X-ray emission are routinely observed around massive galaxies and in galaxy groups and clusters. We study these observational di…