35 citations · 89 across the 3 of their papers we have counts for
5 papers
High-resolution, 3D radiative transfer modelling IV. AGN-powered dust heating in NGC 1068
S. Viaene, A. Nersesian, J. Fritz +18
Dust emission, an important diagnostic of star formation and ISM mass throughout the Universe, can be powered by sources unrelated to ongoing star formation. In the framework of th…
High-resolution, 3D radiative transfer modelling III. The DustPedia barred galaxies
Angelos Nersesian, Sam Verstocken, Sebastien Viaene +17
Context: Dust in late-type galaxies in the local Universe is responsible for absorbing approximately one third of the energy emitted by stars. It is often assumed that dust heating…
High-resolution, 3D radiative transfer modelling. II. The early-type spiral galaxy M81
Sam Verstocken, Angelos Nersesian, Maarten Baes +14
Interstellar dust absorbs stellar light very efficiently and thus shapes the energetic output of galaxies. Studying the impact of different stellar populations on the dust heating…
Reproducing the Universe: a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample
Ana Trčka, Maarten Baes, Peter Camps +17
We compare the spectral energy distributions (SEDs) and inferred physical properties for simulated and observed galaxies at low redshift. We exploit UV-submillimetre mock fluxes of…
The fraction of bolometric luminosity absorbed by dust in DustPedia galaxies
S. Bianchi, P. De Vis, S. Viaene +16
We study the fraction of stellar radiation absorbed by dust, f_abs, in 814 galaxies of different morphological types. The targets constitute the vast majority (93%) of the DustPedi…