most citedAuriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions

10 citations · 38 across the 8 of their papers we have counts for

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astro-ph.GA2024★ 3 cited

Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies

Nora Shipp, Alexander H. Riley, Christine M. Simpson +7

Galaxies like the Milky Way are surrounded by complex populations of satellites at all stages of tidal disruption. In this paper, we present a dynamical study of the disrupting sat…

astro-ph.GA2024

Progenitor diversity in the accreted stellar halos of Milky Way-like galaxies

Sy-Yun Pu, Andrew P. Cooper, Robert J. J. Grand +2

Ongoing large stellar spectroscopic surveys of the Milky Way seek to reconstruct the major events in the assembly history of the Galaxy. Chemical and kinematic observations can be…

astro-ph.GA2024★ 10 cited

Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions

Alexander H. Riley, Nora Shipp, Christine M. Simpson +8

In a hierarchically formed Universe, galaxies accrete smaller systems that tidally disrupt as they evolve in the host's potential. We present a complete catalogue of disrupting gal…

astro-ph.GA2024★ 1 cited

The distant Milky Way halo from the Southern hemisphere: Characterization of the LMC-induced dynamical-friction wake

Manuel Cavieres, Julio Chanamé, Camila Navarrete +6

The infall of the Large Magellanic Cloud (LMC) into the Milky Way's halo impacts the distribution of stars and dark matter in our Galaxy. Mapping the observational consequences of…

astro-ph.GA2024★ 4 cited

Differences in the Physical Properties of Satellite Galaxies within Relaxed and Disturbed Galaxy Groups and Clusters

F. Aldás, Facundo A. Gómez, C. Vega-Martínez +2

Galaxy groups and clusters are the most massive collapsed structures in the Universe. Those structures are formed by collapsing with other smaller structures. Groups and cluster me…

astro-ph.GA2024★ 8 cited

Galaxy evolution in compact groups II. Witnessing the influence of major structures in their evolution

Gissel P. Montaguth, Antonela Monachesi, Sergio Torres-Flores +15

Compact groups (CGs) of galaxies are extreme environments for morphological transformations and the cessation of star formation. Though initially considered isolated, it is now rec…