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...
| Hlavní autoři: | , , , , , , , |
|---|---|
| Médium: | Journal article |
| Vydáno: |
American Astronomical Society
2016
|