Constrained simulation of the bullet cluster

Craig Lage, Glennys Farrar

    Research output: Contribution to journalArticle

    Abstract

    In this work, we report on a detailed simulation of the Bullet Cluster (1E0657-56) merger, including magnetohydrodynamics, plasma cooling, and adaptive mesh refinement. We constrain the simulation with data from gravitational lensing reconstructions and the 0.5-2 keV Chandra X-ray flux map, then compare the resulting model to higher energy X-ray fluxes, the extracted plasma temperature map, Sunyaev-Zel'dovich effect measurements, and cluster halo radio emission. We constrain the initial conditions by minimizing the chi-squared figure of merit between the full two-dimensional (2D) observational data sets and the simulation, rather than comparing only a few features such as the location of subcluster centroids, as in previous studies. A simple initial configuration of two triaxial clusters with Navarro-Frenk-White dark matter profiles and physically reasonable plasma profiles gives a good fit to the current observational morphology and X-ray emissions of the merging clusters. There is no need for unconventional physics or extreme infall velocities. The study gives insight into the astrophysical processes at play during a galaxy cluster merger, and constrains the strength and coherence length of the magnetic fields. The techniques developed here to create realistic, stable, triaxial clusters, and to utilize the totality of the 2D image data, will be applicable to future simulation studies of other merging clusters. This approach of constrained simulation, when applied to well-measured systems, should be a powerful complement to present tools for understanding X-ray clusters and their magnetic fields, and the processes governing their formation.

    Original languageEnglish (US)
    Article number144
    JournalAstrophysical Journal
    Volume787
    Issue number2
    DOIs
    StatePublished - Jun 1 2014

    Fingerprint

    simulation
    plasma
    merger
    magnetic field
    magnetohydrodynamics
    x rays
    plasma cooling
    physics
    radio
    plasma temperature
    cooling
    radio emission
    profiles
    magnetic fields
    figure of merit
    complement
    centroids
    halos
    dark matter
    astrophysics

    Keywords

    • dark matter
    • galaxies: clusters: general
    • galaxies: clusters: intracluster medium
    • magnetic fields
    • magnetohydrodynamics (MHD)
    • methods: numerical

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Constrained simulation of the bullet cluster. / Lage, Craig; Farrar, Glennys.

    In: Astrophysical Journal, Vol. 787, No. 2, 144, 01.06.2014.

    Research output: Contribution to journalArticle

    Lage, Craig ; Farrar, Glennys. / Constrained simulation of the bullet cluster. In: Astrophysical Journal. 2014 ; Vol. 787, No. 2.
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