Skip to main content

Research Repository

Advanced Search

Subhalo destruction in the Apostle and Auriga simulations

Richings, Jack; Frenk, Carlos; Jenkins, Adrian; Robertson, Andrew; Fattahi, Azadeh; Grand, Robert JJ; Navarro, Julio; Pakmor, Rüdiger; Gomez, Facundo A; Marinacci, Federico; Oman, Kyle

Subhalo destruction in the Apostle and Auriga simulations Thumbnail


Authors

Jack Richings

Robert JJ Grand

Julio Navarro

Rüdiger Pakmor

Facundo A Gomez

Federico Marinacci

Kyle Oman



Abstract

N-body simulations make unambiguous predictions for the abundance of substructures within dark matter halos. However, the inclusion of baryons in the simulations changes the picture because processes associated with the presence of a large galaxy in the halo can destroy subhalos and substantially alter the mass function and velocity distribution of subhalos. We compare the effect of galaxy formation on subhalo populations in two state-of-the-art sets of hydrodynamical ΛCDM simulations of Milky Way mass halos, APOSTLE and AURIGA. We introduce a new method for tracking the orbits of subhalos between simulation snapshots that gives accurate results down to a few kiloparsecs from the centre of the halo. Relative to a dark matter-only simulation, the abundance of subhalos in APOSTLE is reduced by 50% near the centre and by 10% within r200. In AURIGA the corresponding numbers are 80% and 40%. The velocity distributions of subhalos are also affected by the presence of the galaxy, much more so in AURIGA than in APOSTLE. The differences on subhalo properties in the two simulations can be traced back to the mass of the central galaxies, which in AURIGA are typically twice as massive as those in APOSTLE. We show that some of the results from previous studies are inaccurate due to systematic errors in the modelling of subhalo orbits near the centre of halos.

Citation

Richings, J., Frenk, C., Jenkins, A., Robertson, A., Fattahi, A., Grand, R. J., …Oman, K. (2020). Subhalo destruction in the Apostle and Auriga simulations. Monthly Notices of the Royal Astronomical Society, 492(4), 5780-5793. https://doi.org/10.1093/mnras/stz3448

Journal Article Type Article
Acceptance Date Dec 4, 2019
Online Publication Date Dec 17, 2019
Publication Date Mar 31, 2020
Deposit Date Jan 3, 2020
Publicly Available Date Jan 3, 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 492
Issue 4
Pages 5780-5793
DOI https://doi.org/10.1093/mnras/stz3448

Files


Accepted Journal Article (689 Kb)
PDF

Copyright Statement
This article has been accepted for publication in the Monthly notices of the Royal Astronomical Society ©: 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





You might also like



Downloadable Citations