The impact of two massive early accretion events in a Milky Way-like galaxy: repercussions for the buildup of the stellar disc and halo

Orkney, Matthew D. A., Laporte, Chervin F. P., Grand, Robert J. J., Gómez, Facundo A., van de Voort, Freeke ORCID: https://orcid.org/0000-0002-6301-638X, Marinacci, Federico, Fragkoudi, Francesca, Pakmor, Ruediger and Springel, Volker 2022. The impact of two massive early accretion events in a Milky Way-like galaxy: repercussions for the buildup of the stellar disc and halo. Monthly Notices of the Royal Astronomical Society: Letters 517 (1) , L138–L142. 10.1093/mnrasl/slac126

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Abstract

We identify and characterize a Milky Way-like realization from the Auriga simulations with two consecutive massive mergers ∼2  Gyr apart at high redshift, comparable to the reported Kraken and Gaia-Sausage-Enceladus. The Kraken-like merger (z = 1.6, MTot=8×1010M⊙ ⁠) is gas-rich, deposits most of its mass in the inner 10  kpc, and is largely isotropic. The Sausage-like merger (z = 1.14, MTot=1×1011M⊙ ⁠) leaves a more extended mass distribution at higher energies, and has a radially anisotropic distribution. For the higher-redshift merger, the stellar mass ratio of the satellite to host galaxy is high (1:3). As a result, the chemistry of the remnant is indistinguishable from contemporaneous in situ populations, making it challenging to identify through chemical abundances. This naturally explains why all abundance patterns attributed so far to Kraken are in fact fully consistent with the metal-poor in situ so-called Aurora population and thick disc. However, our model makes a falsifiable prediction: if the Milky Way underwent a gas-rich double merger at high redshift, then this should be imprinted on its star formation history with bursts about ∼2  s apart. This may offer constraining power on the highest-redshift massive mergers.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Publisher:	Oxford University Press
ISSN:	1745-3933
Date of First Compliant Deposit:	3 February 2023
Date of Acceptance:	10 October 2022
Last Modified:	03 May 2023 07:55
URI:	https://orca.cardiff.ac.uk/id/eprint/156481

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