Differences
This shows you the differences between two versions of the page.
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sim:gallery [2017/12/04 12:41] leo created |
sim:gallery [2018/10/05 15:46] (current) leo |
| === AGN simulations (by Leo, Nov 2017) === | === AGN simulations with the old simulator (by Leo, Nov 2017) === |
| We processed the hydro/radiative transfer AGN simulations by Schartmann et al. 2014 through various versions of the METIS simulator in the month of November 2017. The model was intended to show the circum-nuclear material on parsec scale (for comparisons with VLTI observations) and the original pixel scale was increased 10x so that a pixel corresponded to 2 milli-arcseconds. This is astronomically "allowed" as the total extent of the AGN-heated dust is much larger than what is seen by VLTI and is expected to look similarly filamentary on larger scales. This is what the model image looks like (left: log scaled; right: sqrt scaled, FoV: 0.6" x 0.6"): | We processed the hydro/radiative transfer AGN simulations by Schartmann et al. 2014 through various versions of the METIS simulator in the month of November 2017. The model was intended to show the circum-nuclear material on parsec scale (for comparisons with VLTI observations) and the original pixel scale was increased 10x so that a pixel corresponded to 2 milli-arcseconds. This is astronomically "allowed" as the total extent of the AGN-heated dust is much larger than what is seen by VLTI and is expected to look similarly filamentary on larger scales. This is what the model image looks like (left: log scaled; right: sqrt scaled, FoV: 0.6" x 0.6"): |
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