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VINTERGATAN-GM: How do mergers affect the satellite populations of MW-like galaxies?

Joshi, Gandhali D; Pontzen, Andrew; Agertz, Oscar; Rey, Martin P; Read, Justin; Renaud, Florent; (2024) VINTERGATAN-GM: How do mergers affect the satellite populations of MW-like galaxies? Monthly Notices of the Royal Astronomical Society , 528 (2) pp. 2346-2357. 10.1093/mnras/stae129. Green open access

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Abstract

We investigate the impact of a galaxy’s merger history on its system of satellites using the new VINTERGATAN-GM suite of zoom-in hydrodynamical simulations of Milky Way-mass systems. The suite simulates five realizations of the same halo with targeted ‘genetic modifications’ (GMs) of a z ≈ 2 merger, but resulting in the same halo mass at z = 0. We find that differences in the satellite stellar mass functions last for 2.25 − 4.25 Gyr after the z ≈ 2 merger; specifically, the haloes that have undergone smaller mergers host up to 60% more satellites than those of the larger merger scenarios. However, by z = 0 these differences in the satellite stellar mass functions have been erased. The differences in satellite numbers seen soon after the mergers are driven by several factors, including the timings of significant mergers (with M200c mass ratios >1 : 30 and bringing in M* ≥ 108M⊙ at infall), the masses and satellite populations of the central and merging systems, and the subsequent extended history of smaller mergers. The results persist when measured at fixed central stellar mass rather than fixed time, implying that a host’s recent merger history can be a significant source of scatter when reconstructing its dynamical properties from its satellite population.

Type: Article
Title: VINTERGATAN-GM: How do mergers affect the satellite populations of MW-like galaxies?
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stae129
Publisher version: http://dx.doi.org/10.1093/mnras/stae129
Language: English
Additional information: Copyright © The Author(s) 2024. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
Keywords: Galaxies: dwarf, galaxies: formation, galaxies: evolution, galaxies: interactions
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10186045
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