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...
| প্রধান লেখক: | , , , , , , , |
|---|---|
| বিন্যাস: | Journal article |
| প্রকাশিত: |
American Astronomical Society
2016
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