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Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at
Yuan-Ming Hsu, Hiroyuki Hirashita, Yen-Hsing Lin +2
Dust emission from high-redshift galaxies gives us a clue to the origin and evolution of dust in the early Universe. Previous studies have shown that different sources of dust (ste…
The resolved scaling relations in DustPedia: Zooming in on the local Universe
Viviana Casasola, Simone Bianchi, Laura Magrini +18
We perform a homogeneous analysis of an unprecedented set of spatially resolved scaling relations (SRs) between ISM components and other properties in the range of scales 0.3-3.4 k…
MIGHTEE-HI: The HI mass-stellar mass relation over the last billion years
Hengxing Pan, Matt J. Jarvis, Mario G. Santos +19
We study the relation over the last billion years using the MIGHTEE-HI sample. We first model the upper envelope of the relation with…
The Einasto model for dark matter haloes
Maarten Baes
Context: The Einasto model has become one of the most popular models for describing the density profile of dark matter haloes. There have been relatively few comprehensive studies…
UV to submillimetre luminosity functions of TNG50 galaxies
Ana Trcka, Maarten Baes, Peter Camps +7
We apply the radiative transfer (RT) code SKIRT on a sample of ~14000 low-redshift (z<= 0.1) galaxies extracted from the TNG50 simulation to enable an apples-to-apples comparison w…
Monte Carlo radiative transfer with explicit absorption to simulate absorption, scattering, and stimulated emission
Maarten Baes, Peter Camps, Kosei Matsumoto
Context: The Monte Carlo method is probably the most widely used approach to solve the radiative transfer problem, especially in a general 3D geometry. The physical processes of em…