activity
20172026
most citedVINTERGATAN I: The origins of chemically, kinematically and structurally distinct discs in a simulated Milky Way-mass galaxy

170 citations · 1.3k across the 49 of their papers we have counts for

collaborators
Showing 2023Show all

9 papers · 1 filter

astro-ph.GA2023★ 3 cited

From particles to orbits: precise dark matter density profiles using dynamical information

Claudia Muni, Andrew Pontzen, Jason L. Sanders +3

We introduce a new method to calculate dark matter halo density profiles from simulations. Each particle is 'smeared' over its orbit to obtain a dynamical profile that is averaged…

astro-ph.GA2023

EDGE -- Dark matter or astrophysics? Breaking dark matter heating degeneracies with HI rotation in faint dwarf galaxies

Martin P. Rey, Matthew D. A. Orkney, Justin I. Read +6

Low-mass dwarf galaxies are expected to reside within dark matter haloes that have a pristine, `cuspy' density profile within their stellar half-light radii. This is because they f…

astro-ph.GA2023

EDGE: The direct link between mass growth history and the extended stellar haloes of the faintest dwarf galaxies

Alex Goater, Justin I. Read, Noelia E. D. Noël +9

Ultra-faint dwarf galaxies (UFDs) are commonly found in close proximity to the Milky Way and other massive spiral galaxies. As such, their projected stellar ellipticity and extende…

astro-ph.GA2023★ 1 cited

VINTERGATAN-GM: How do mergers affect the satellite populations of MW-like galaxies?

Gandhali D. Joshi, Andrew Pontzen, Oscar Agertz +3

We investigate the impact of a galaxy's merger history on its system of satellites using the new \textsc{vintergatan-gm} suite of zoom-in hydrodynamical simulations of Milky Way-ma…

astro-ph.GA2023★ 7 cited

The Highest-Redshift Balmer Breaks as a Test of CDM

Charles L. Steinhardt, Albert Sneppen, Thorbjørn Clausen +3

Recent studies have reported tension between the presence of luminous, high-redshift galaxies and the halo mass functions predicted by standard cosmology. Here, an improved test is…

astro-ph.GA2023★ 151 cited

Nitrogen enhancements 440 Myr after the Big Bang: super-solar N/O, a tidal disruption event or a dense stellar cluster in GN-z11?

Alex J. Cameron, Harley Katz, Martin P. Rey +1

Recent observations of GN-z11 with JWST/NIRSpec revealed numerous oxygen, carbon, nitrogen, and helium emission lines at . Using the measured line fluxes, we derive abundan…

astro-ph.GA2023★ 16 cited

EDGE: The shape of dark matter haloes in the faintest galaxies

Matthew D. A. Orkney, Ethan Taylor, Justin I. Read +5

Collisionless Dark Matter Only (DMO) structure formation simulations predict that Dark Matter (DM) haloes are prolate in their centres and triaxial towards their outskirts. The add…

astro-ph.GA2023★ 27 cited

Boosting galactic outflows with enhanced resolution

Martin P. Rey, Harley B. Katz, Alex J. Cameron +2

We study how better resolving the cooling length of galactic outflows affect their energetics. We perform radiative-hydrodynamical galaxy formation simulations of an isolated dwarf…

astro-ph.SR2023★ 10 cited

Bringing Stellar Evolution & Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022

Sam Geen, Poojan Agrawal, Paul A. Crowther +34

Stars strongly impact their environment, and shape structures on all scales throughout the universe, in a process known as ``feedback''. Due to the complexity of both stellar evolu…