most citedThe COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution

25 citations · 33 across the 3 of their papers we have counts for

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astro-ph.GA20265 cited

COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase

Evgenii Chaikin, Joop Schaye, Matthieu Schaller +17

We present the calibration of stellar and active galactic nucleus (AGN) feedback in the subgrid model for the new COLIBRE hydrodynamical simulations of galaxy formation. COLIBRE di…

astro-ph.GA202625 cited

The COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution

Joop Schaye, Evgenii Chaikin, Matthieu Schaller +18

We present the COLIBRE galaxy formation model and the COLIBRE suite of cosmological hydrodynamical simulations. COLIBRE includes new models for radiative cooling, dust grains, star…

astro-ph.GA20263 cited

The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles

Kris Walker, Aaron Ludlow, Chris Power +2

We examine the splashback structure of galaxy clusters using hydrodynamical simulations from the GIZMO run of The Three Hundred Project, focusing on the relationship between the st…

astro-ph.GA2025

The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies

Katy L. Proctor, Aaron D. Ludlow, Claudia del P. Lagos +1

Stellar haloes form through the disruption of satellite galaxies over time, making them a promising observable for constraining galaxy merger histories. We use a dynamical decompos…

astro-ph.GA2024

Supermassive black hole feedback quenches disc galaxies and suppresses bar formation in TNG50

Matthew Frosst, Danail Obreschkow, Aaron Ludlow +2

We use the cosmological magneto-hydrodynamical simulation TNG50 to study the relationship between black hole feedback, the presence of stellar bars, and star formation quenching in…

astro-ph.GA2024

The active role of co-evolving haloes in stellar bar formation

Matthew Frosst, Danail Obreschkow, Aaron D. Ludlow

We use idealised N-body simulations of equilibrium discs in live and static haloes to study how dark matter co-evolution impacts the assembly of stellar particles into a bar and th…