The formation of entropy cores in non-radiative galaxy cluster simulations: Smoothed particle hydrodynamics versus adaptive mesh refinement

Chris Power, J.I. Read, A. Hobbs

    Research output: Contribution to journalArticle

    22 Citations (Scopus)
    151 Downloads (Pure)
    Original languageEnglish
    Pages (from-to)3243-3256
    Number of pages14
    JournalMonthly Notices of the Royal Astronomical Society
    Volume440
    Issue number4
    Early online date17 Apr 2014
    DOIs
    Publication statusPublished - 1 Jun 2014

    Cite this

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    title = "The formation of entropy cores in non-radiative galaxy cluster simulations: Smoothed particle hydrodynamics versus adaptive mesh refinement",
    author = "Chris Power and J.I. Read and A. Hobbs",
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    T1 - The formation of entropy cores in non-radiative galaxy cluster simulations: Smoothed particle hydrodynamics versus adaptive mesh refinement

    AU - Power, Chris

    AU - Read, J.I.

    AU - Hobbs, A.

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    DO - 10.1093/mnras/stu418

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    EP - 3256

    JO - Monthly Notices of the Royal Astronomical Society

    JF - Monthly Notices of the Royal Astronomical Society

    SN - 0035-8711

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    ER -