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19962023
most citedThe Graininess of Dark Matter Haloes

76 citations · 367 across the 14 of their papers we have counts for

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Showing 2018Show all

7 papers · 1 filter

astro-ph.GA2018

The large-scale structure of the halo of the Andromeda galaxy II. Hierarchical structure in the Pan-Andromeda Archaeological Survey

Alan W. McConnachie, Rodrigo Ibata, Nicolas Martin +29

The Pan-Andromeda Archaeological Survey is a survey of square degrees centered on the Andromeda (M31) and Triangulum (M33) galaxies that has provided the most extensive pano…

astro-ph.GA2018

Can Stellar Discs in a Cosmological Setting Avoid Forming Strong Bars?

Jacob S. Bauer, Lawrence M. Widrow

We investigate the connection between the vertical structure of stellar discs and the formation of bars using high-resolution simulations of galaxies in isolation and in the cosmol…

astro-ph.GA2018

Simulating non-axisymmetric flows in disc galaxies

T. H. Randriamampandry, N. Deg, C. Carignan +1

We present a two-step method to simulate and study non-circular motions in strongly barred galaxies. The first step is to constrain the initial parameters using a Bayesian analysis…

astro-ph.GA2018

Emergence of the Gaia Phase Space Spirals from Bending Waves

Keir Darling, Lawrence M. Widrow

We discuss the physical mechanism by which pure vertical bending waves in a stellar disc evolve to form phase space spirals similar to those discovered by Antoja et al. ( arXiv:180…

astro-ph.GA2018

Formation of LISA Black Hole Binaries in Merging Dwarf Galaxies: the Imprint of Dark Matter

Tomas Tamfal, Pedro R. Capelo, Stelios Kazantzidis +4

Theoretical models for the expected merger rates of intermediate-mass black holes (IMBHs) are vital for planned gravitational-wave detection experiments such as the Laser Interfero…

astro-ph.GA2018

Bending Waves in the Milky Way's disc from halo substructure

Matthew H. Chequers, Lawrence M. Widrow, Keir Darling

We use -body simulations to investigate the excitation of bending waves in a Milky Way-like disc-bulge-halo system. The dark matter halo consists of a smooth component and a pop…