activity
20172024
most citedA trail of dark matter-free galaxies from a bullet dwarf collision

97 citations · 199 across the 9 of their papers we have counts for

collaborators

12 papers

astro-ph.GA20242 cited

The cosmic globular cluster formation history in the E-MOSAICS simulations

Philipp S. Joschko, J. M. Diederik Kruijssen, Sebastian Trujillo-Gomez +4

We present a comprehensive analysis of globular cluster (GC) formation and evolution across the Mpc volume of the E-MOSAICS galaxy formation simulations. Defining GCs as…

astro-ph.GA202297 cited

A trail of dark matter-free galaxies from a bullet dwarf collision

Pieter van Dokkum, Zili Shen, Michael A. Keim +8

The ultra-diffuse galaxies DF2 and DF4 in the NGC1052 group share several unusual properties: they both have large sizes, rich populations of overluminous and large globular cluste…

astro-ph.GA20221 cited

Constraining the shape of dark matter haloes with globular clusters

Marta Reina-Campos, Sebastian Trujillo-Gomez, Joel L. Pfeffer +4

We explore how diffuse stellar light and globular clusters (GCs) can be used to trace the matter distribution of their host halo using an observational methodology. For this, we us…

astro-ph.GA202116 cited

Using cosmological simulations and synthetic absorption spectra to assess the accuracy of observationally derived CGM metallicities

Rachel Marra, Christopher W. Churchill, Caitlin Doughty +6

We used adaptive mesh refinement hydrodynamic cosmological simulations of a Milky Way-type galaxy and a Dwarf galaxy and generated synthetic quasar absorption-line spec…

astro-ph.GA20218 cited

What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies

Meghan E. Hughes, Prashin Jethwa, Michael Hilker +8

Dynamical models allow us to connect the motion of a set of tracers to the underlying gravitational potential, and thus to the total (luminous and dark) matter distribution. They a…

astro-ph.GA202040 cited

Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations

Benjamin W. Keller, J. M. Diederik Kruijssen, Joel Pfeffer +5

Globular clusters (GCs) are typically old, with most having formed at z >~ 2. This makes understanding their birth environments difficult, as they are typically too distant to obse…