activity
20242026
most citedThe mass distribution in and around the Local Group

1 citations · 1 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Alignment of the Milky Way and M31 with their cosmic environment. New insights from constrained Local Group simulations

Hanneke C. Woudenberg, Amina Helmi, Ewoud Wempe +4

The large-scale environment is thought to play an important role in setting galaxy properties. The Milky Way (MW) and Andromeda (M31) reside in the Local Group, embedded in the Loc…

astro-ph.GA2026

The capture of halo material by orbiting subhaloes

Hang Yang, Simon D. M. White, Liang Gao

When a dark matter halo falls into a more massive object and becomes a subhalo, it typically loses much of its mass through tidal stripping. The reverse process is also possible in…

astro-ph.GA20261 cited

The mass distribution in and around the Local Group

Ewoud Wempe, Simon D. M. White, Amina Helmi +2

Our Galaxy, Andromeda and their companion dwarf galaxies form the Local Group. Most of the mass in and around it is believed to be dark matter rather than gas or stars, so its dist…

astro-ph.GA2025

The effect of environment on the mass assembly history of the Milky Way and M31

Ewoud Wempe, Amina Helmi, Simon D. M. White +2

We study the mass growth histories of the halos of Milky Way and M31 analogues formed in constrained cosmological simulations of the Local Group. These simulations constitute a fai…

astro-ph.GA2024

Constrained cosmological simulations of the Local Group using Bayesian hierarchical field-level inference

Ewoud Wempe, Guilhem Lavaux, Simon D. M. White +3

We present a novel approach based on Bayesian field-level inference capable of resolving individual galaxies within the Local Group (LG), enabling detailed studies of its structure…