most citedThe Milky Way - Large Magellanic Cloud Interaction with Simulation Based Inference

3 citations · 3 across the 2 of their papers we have counts for

collaborators

10 papers

astro-ph.GA20263 cited

The Milky Way - Large Magellanic Cloud Interaction with Simulation Based Inference

Richard A. N. Brooks, Jason L. Sanders, Vedant Chandra +4

The infall of the Large Magellanic Cloud (LMC) into the Milky Way (MW) has displaced the MW's centre of mass, manifesting as an observed reflex motion in the velocities of outer ha…

astro-ph.GA2026

Bar-induced migration of Centauri away from Gaia Sausage-Enceladus

Adam M. Dillamore, Hanyuan Zhang, Vasily Belokurov

The globular cluster Cen has been suggested to have originated in the Gaia Sausage-Enceladus (GSE) merger event, possibly as its nuclear star cluster. However, the present-day…

astro-ph.GA2026

Quantifying the Milky Way, LMC and their interaction using all-sky kinematics of outer halo stars

Richard A. N. Brooks, Jason L. Sanders, Adam M. Dillamore +4

The recent pericentric passage of the Large Magellanic Cloud (LMC) has dislodged the Milky Way's (MW) centre of mass, inducing dynamical disequilibrium, the reflex motion, in the k…

astro-ph.GA2026

GSE vs. LMC: reshaping of radially biased stellar haloes by satellites

Adam M. Dillamore, Jason L. Sanders, Richard A. N. Brooks

Perturbations from the Large Magellanic Cloud (LMC) of the Milky Way's stellar and dark matter haloes are well-established. However, studies have generally not considered the high…

astro-ph.GA2026

The erasure of Galactic bar resonances by dark matter subhaloes

Elliot Y. Davies, Adam M. Dillamore, Vasily Belokurov +1

In the context of increasing appreciation for the coupling between the Galactic bar and the halo, we introduce a new framework using stars trapped in resonance with the bar to prob…

astro-ph.GA2026

Geometry of the Milky Way's dark matter from dynamical models of the tilted stellar halo

Adam M. Dillamore, Jason L. Sanders

The shape and orientation of the Milky Way's dark matter halo remain poorly constrained. Observations of the accreted stellar halo show that it is triaxial and tilted with respect…