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

doi:10.1093/mnras/stu418

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

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Original language	English
Pages (from-to)	3243-3256
Number of pages	14
Journal	Monthly Notices of the Royal Astronomical Society
Volume	440
Issue number	4
Early online date	17 Apr 2014
DOIs	https://doi.org/10.1093/mnras/stu418
Publication status	Published - 1 Jun 2014

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This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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Cite this

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