Comparing simulations of AGN feedback
We perform adaptive mesh refinement (AMR) and smoothed particle hydrodynamics (SPH) cosmological zoom simulations of a region around a forming galaxy cluster, comparing the ability of the methods to handle successively more complex baryonic physics. In the simplest, non-radiative case, the two metho...
| Main Authors: | , , , , , , , |
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| 格式: | Journal article |
| 出版: |
American Astronomical Society
2016
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