activity
19982023
most citedBeasts of the Southern Wild: Discovery of nine Ultra Faint satellites in the vicinity of the Magellanic Clouds

552 citations · 4.6k across the 73 of their papers we have counts for

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Showing 2022 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2022★ 4 cited

A correlation between accreted stellar kinematics and dark matter halo spin in the ARTEMIS simulations

Adam M. Dillamore, Vasily Belokurov, N. Wyn Evans +1

We report a correlation between the presence of a Gaia-Sausage-Enceladus (GSE) analogue and dark matter halo spin in the ARTEMIS simulations of Milky Way-like galaxies. The haloes…

astro-ph.GA2022

Chemical and stellar properties of early-type dwarf galaxies around the Milky Way

Vasily Belokurov, N. Wyn Evans

Early-type dwarfs (ETDs) are the end points of the evolution of low-mass galaxies whose gas supply has been extinguished. The cessation of star-formation lays bare the ancient stel…

astro-ph.GA2022★ 1 cited

Milky Way's eccentric constituents with , APOGEE GALAH

G. C. Myeong, Vasily Belokurov, David S. Aguado +3

We report the results of an unsupervised decomposition of the local stellar halo in the chemo-dynamical space spanned by the abundance measurements from APOGEE DR17 and GALAH DR3.…

astro-ph.GA2022★ 28 cited

The impact of a massive Sagittarius dSph on GD-1-like streams

Adam M. Dillamore, Vasily Belokurov, N. Wyn Evans +1

We investigate the effects of a massive () Sagittarius dwarf spheroidal galaxy (Sgr) on stellar streams using test particle simulations in a realistic…

astro-ph.GA2022★ 37 cited

The Local Group Mass in the light of Gaia

David Benisty, Eugene Vasiliev, N. Wyn Evans +3

High accuracy proper motions (PMs) of M31 and other Local Group satellites have now been provided by the {\it Gaia} satellite. We revisit the Timing Argument to compute the total m…

astro-ph.GA2022★ 17 cited

Mass Segregation in the Hyades Cluster

N. Wyn Evans, Semyeong Oh

Using the Gaia colour-magnitude diagram, we assign masses to a catalogue of 979 confirmed members of the Hyades cluster and tails. By fitting the cumulative mass profile, stars wit…