activity
20062026
most citedFundamental differences between SPH and grid methods

623 citations · 7.6k across the 126 of their papers we have counts for

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114 papers · 1 filter

astro-ph.GA2026

EDGE-INFERNO: The chemical signatures of assembly history in reionization fossils

Eric P. Andersson, Martin P. Rey, Alexander P. Ji +9

In galaxies, stellar populations represent a superposition of both in situ and accreted components, tracing internal chemical evolution as well as the histories of merged satellite…

astro-ph.GA2026

Early onset of the hot circumgalactic medium around Milky Way galaxies

Víctor Rufo-Pastor, Oscar Agertz, Santi Roca-Fábrega +6

Hot coronae are key regulators in Milky Way (MW)-type galaxy formation and are thought to emerge once a galaxy's dark matter halo crosses a critical mass threshold, $M_{\mathrm{vir…

astro-ph.GA2026

The driving mode of turbulence in disc galaxy simulations with adaptive mesh refinement

James Watt, Christoph Federrath, Thorsten Tepper-Garcia +2

Turbulence is a key ingredient in controlling the structure of the interstellar medium (ISM) and star formation, yet we still lack a detailed understanding of its drivers in galaxi…

astro-ph.GA2026

Nexus-CDM: Isolated Galaxy Simulations with Cosmologically Evolving Dark-Matter Halos I. Method and Validation

Thor Tepper-García, Joss Bland-Hawthorn, Oscar Agertz +1

Galaxy evolution can be modelled in two complementary ways. Standalone simulations place a single galaxy in isolation, evolving it under controlled initial conditions without the s…

astro-ph.GA2026

Turbulent gas-rich discs at high redshift: the origin of early massive stellar bars

Joss Bland-Hawthorn, Thor Tepper-Garcia, Chris Hamilton +4

Recent observations combining the power of ALMA and JWST have revealed large ( kpc), massive () stellar bars at when the Universe…

astro-ph.GA2026

Magnetic destabilisation in disc galaxies: Filament/feather formation

Raghav Arora, Oscar Agertz, Christoph Federrath +1

Gas gravitational instability plays a crucial role in secular galactic evolution, but the role played by magnetic fields in mediating this instability - despite their dynamical rel…