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The AGN dusty torus as a clumpy two-phase medium: radiative transfer modeling with SKIRT
Marko Stalevski, Jacopo Fritz, Maarten Baes +1
We modeled the AGN dusty torus as a clumpy two-phase medium, with high-density clumps embedded in a low-density interclump dust. To obtain spectral energy distributions and images…
Gravitational microlensing of AGN dusty tori
Marko Stalevski, Predrag Jovanović, Luka Č. Popović +1
We investigated the gravitational microlensing of active galactic nucleus dusty tori in the case of lensed quasars in the infrared domain. The dusty torus is modeled as a clumpy tw…
AGN Dusty Tori as a Clumpy Two-Phase Medium: The 10 Micron Silicate Feature
Marko Stalevski, Jacopo Fritz, Maarten Baes +2
We investigated the emission of active galactic nuclei dusty tori in the infrared domain, with a focus on the 10 micron silicate feature. We modeled the dusty torus as a clumpy two…
Three-dimensional radiative transfer modeling of AGN dusty tori as a clumpy two-phase medium
Marko Stalevski, Jacopo Fritz, Maarten Baes +2
We investigate the emission of active galactic nuclei (AGN) dusty tori in the infrared domain. Following theoretical predictions coming from hydrodynamical simulations, we model th…
Efficient 3D NLTE dust radiative transfer with SKIRT
Maarten Baes, Joris Verstappen, Ilse De Looze +5
We present an updated version of SKIRT, a 3D Monte Carlo radiative transfer code developed to simulate dusty galaxies. The main novel characteristics of the SKIRT code are the use…
The complex interplay of dust and star light in spiral galaxy discs
Maarten Baes, Dimitri Gadotti, Joris Verstappen +4
Interstellar dust grains efficiently absorb and scatter UV and optical radiation in galaxies, and therefore can significantly affect the apparent structure of spiral galaxies. We d…