Resilience of sloshing cold fronts against subsequent minor mergers

Author:

Vaezzadeh Iraj1ORCID,Roediger Elke1,Cashmore Claire1,Hunt Matthew1,ZuHone John2,Forman William2,Jones Christine2,Kraft Ralph2,Nulsen Paul23,Su Yuanyuan4ORCID,Churazov Eugene56

Affiliation:

1. E.A. Milne Centre, University of Hull , Cottingham Road, Hull HU6 7RX, UK

2. Smithsonian Astrophysical Observatory, Harvard-Smithsonian Center for Astrophysics , 60 Garden St., Cambridge, MA 02138, USA

3. Physics and Astronomy, University of Kentucky , 505 Rose street, Lexington, KY 40506, USA

4. ICRAR, University of Western Australia , 35 Stirling Hwy, Crawley, WA 6009, Australia

5. Max Planck Institute for Astrophysics , Karl-Schwarzschild-Str 1, D-85741 Garching, Germany

6. Space Research Institute (IKI) , Profsoyuznaya 84/32, Moscow 117997, Russia

Abstract

ABSTRACT Minor mergers are common in galaxy clusters. They have the potential to create sloshing cold fronts (SCFs) in the intracluster medium of the cluster. However, the resilience of SCFs to subsequent minor mergers is unknown. Here we investigate the extent to which SCFs established by an off-axis minor merger are disrupted by a subsequent minor merger. We perform a suite of 13 hydrodynamic + N-body simulations of idealized triple cluster mergers in which we vary the approach direction and impact parameter of the tertiary cluster. Except for ∼1 Gyr after the first core passage of the tertiary cluster, clear SCFs are present in all merger configurations. Subsequent head-on minor mergers reduce the number of SCFs significantly, while subsequent off-axis minor mergers only moderately reduce the number of SCFs. In particular, outer ($\gtrapprox 500\,$kpc) SCFs are resilient. The results of this work indicate that SCFs are easily formed in the course of a minor merger and are long-lived even if a further minor merger takes place. SCFs thus should be ubiquitous, but deriving the merger history of a given cluster based on its observed SCFs might be more complex than previously thought.

Funder

NASA

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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1. Observational Predictions for the Survival of Atomic Hydrogen in Simulated Fornax-like Galaxy Clusters;The Astrophysical Journal;2024-06-26

2. A toy model for gas sloshing in galaxy clusters;Monthly Notices of the Royal Astronomical Society;2024-02-28

3. The effect of cluster dynamical state on ram-pressure stripping;Monthly Notices of the Royal Astronomical Society;2023-10-01

4. Quasi-spiral solution to the mixed intracluster medium and the universal entropy profile of galaxy clusters;Monthly Notices of the Royal Astronomical Society;2023-04-07

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