We review the recent theoretical and observational developments concerning the interaction
of the Large Magellanic Cloud (LMC) with the Milky Way and its neighbourhood. An …

Abstract We describe the Milky Way Survey (MWS) that will be undertaken with the Dark
Energy Spectroscopic Instrument (DESI) on the Mayall 4 m telescope at the Kitt Peak …

We present a 6D map of the Orphan–Chenab (OC) stream by combining the data from
Southern Stellar Stream Spectroscopic Survey (S 5) and Gaia. We reconstruct the proper …

We report the kinematic, orbital, and chemical properties of 12 stellar streams with no
evident progenitors using line-of-sight velocities and metallicities from the Southern Stellar …

It has recently been shown that the Large Magellanic Cloud (LMC) has a substantial effect
on the Milky Way's stellar halo and stellar streams. Here, we explore how deformations of …

We present Symphony, a compilation of 262 cosmological, cold-dark-matter-only zoom-in
simulations spanning four decades of host halo mass, from 10 11–10 15 M⊙. This …

The ongoing interaction between the Milky Way (MW) and its largest satellite–the Large
Magellanic Cloud (LMC)–creates a significant perturbation in the distribution and kinematics …

Abstract The Magellanic Stream (MS)—an enormous ribbon of gas spanning 140 of the
southern sky trailing the Magellanic Clouds—has been exquisitely mapped in the five …

We present the first detailed comparison of populations of dwarf galaxy stellar streams in
cosmological simulations and the Milky Way. In particular, we compare streams identified …

The non-linear process of cosmic structure formation produces gravitationally bound
overdensities of dark matter known as halos. The abundances, density profiles, ellipticities …