activity
20162024
most citedEDGE: Two routes to dark matter core formation in ultra-faint dwarfs

60 citations · 244 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2024★ 3 cited

One Stream or Two -- Exploring Andromeda's North West Stream

Janet Preston, Denis Erkal, Michelle L. M. Collins +3

We present results of our dynamical stream modelling for the North West Stream in the outer halo of the Andromeda galaxy (M31). Comprising two main segments, the North West Stream…

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.GA2022★ 10 cited

EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf

Matthew D. A. Orkney, Justin I. Read, Oscar Agertz +6

The Eridanus II (EriII) 'ultra-faint' dwarf has a large () and low mass () star cluster (SC) offset from its centre by $23\pm3\,\text{…

astro-ph.GA2021★ 60 cited

EDGE: Two routes to dark matter core formation in ultra-faint dwarfs

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

In the standard Lambda cold dark matter paradigm, pure dark matter simulations predict dwarf galaxies should inhabit dark matter haloes with a centrally diverging density `cusp'. T…

astro-ph.GA2020★ 42 cited

Formation of the largest galactic cores through binary scouring and gravitational wave recoil

Imran Nasim, Alessia Gualandris, Justin I. Read +3

Massive elliptical galaxies are typically observed to have central cores in their projected radial light profiles. Such cores have long been thought to form through `binary scourin…

astro-ph.GA2020★ 31 cited

Defeating stochasticity: coalescence timescales of massive black holes in galaxy mergers

Imran Nasim, Alessia Gualandris, Justin Read +3

The coalescence of massive black hole binaries (BHBs) in galactic mergers is the primary source of gravitational waves (GWs) at low frequencies. Current estimates of GW detection r…

astro-ph.GA2019★ 13 cited

Uncovering the Orbit of the Hercules Dwarf Galaxy

Alexandra L. Gregory, Michelle L. M. Collins, Denis Erkal +6

We present new chemo--kinematics of the Hercules dwarf galaxy based on Keck II-- DEIMOS spectroscopy. Our 21 confirmed members have a systemic velocity of $v_{\mathrm{Herc}}=46.4\p…

astro-ph.GA2019★ 8 cited

A Dwarf Disrupting -- Andromeda XXVII and the North West Stream

Janet Preston, Michelle L. M. Collins, Rodrigo A. Ibata +10

We present a kinematic and spectroscopic analysis of 38 red giant branch stars, in 7 fields, spanning the dwarf spheroidal galaxy Andromeda XXVII and the upper segment of the North…

astro-ph.GA2017★ 48 cited

Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II

Filippo Contenta, Eduardo Balbinot, James A. Petts +6

We present a new technique to probe the central dark matter (DM) density profile of galaxies that harnesses both the survival and observed properties of star clusters. As a first a…

astro-ph.GA2016★ 13 cited

An efficient positive potential-density pair expansion for modelling galaxies

Armando Rojas-Niño, Justin I. Read, Luis Aguilar +1

We present a novel positive potential-density pair expansion for modelling galaxies, based on the Miyamoto-Nagai (MN) disc. By using three sets of such discs, each one of them alig…