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How Unusual is the Milky Way’s Assembly History?

Evans, Tilly A; Fattahi, Azadeh; Deason, Alis J; Frenk, Carlos S

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Authors



Abstract

In the ΛCDM model of structure formation galactic haloes build up by accretion of mass and mergers of smaller haloes. The most recent massive merger event experienced by the Milky Way (MW) halo was the accretion of the Large Magellanic Cloud (LMC; which has a stellar mass of ∼ 109M⊙). Recent analyses of galactic stellar data from the Gaia satellite have uncovered an earlier massive accretion event, the Gaia-Enceladus Sausage (GES), which merged with the MW around 10 Gyr ago. Here, we use the EAGLE cosmological hydrodynamics simulation to study properties of simulated MW-mass haloes constrained to have accretion histories similar to that of the MW, specifically the recent accretion of an “LMC” galaxy and a “GES” merger, with a quiescent period between the GES merger and the infall of the LMC (the “LMC & GES” category). We find that ∼16 per cent of MW-mass haloes have an LMC; ∼5 per cent have a GES event and no further merger with an equally massive object since z = 1; and only 0.65 per cent belong to the LMC & GES category. The progenitors of the MWs in this last category are much less massive than average at early times but eventually catch up with the mean. The LMC & GES category of galaxies naturally end up in the “blue cloud” in the colour-magnitude diagram at z = 0, tend to have a disc morphology and have a larger than average number of satellite galaxies.

Citation

Evans, T. A., Fattahi, A., Deason, A. J., & Frenk, C. S. (2020). How Unusual is the Milky Way’s Assembly History?. Monthly Notices of the Royal Astronomical Society, 497(4), 4311-4321. https://doi.org/10.1093/mnras/staa2202

Journal Article Type Article
Acceptance Date Jul 22, 2020
Online Publication Date Jul 29, 2020
Publication Date 2020-10
Deposit Date Jul 30, 2020
Publicly Available Date Sep 18, 2020
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 497
Issue 4
Pages 4311-4321
DOI https://doi.org/10.1093/mnras/staa2202
Public URL https://durham-repository.worktribe.com/output/1295675

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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.






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