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Modelling the cold dust in nearby spiral galaxies with radiative transfer
Angelos Nersesian, Maarten Baes, Suzanne C. Madden
Cosmic dust grains are one of the fundamental ingredients of the interstellar medium (ISM). In spite of their small contribution to the total mass budget, dust grains play a signif…
Predicting far-infrared maps of galaxies via machine learning techniques
Wouter Dobbels, Maarten Baes
The ultraviolet (UV) to sub-millimetre (submm) spectral energy distribution of galaxies can be roughly divided into two sections: the stellar emission (attenuated by dust) at UV to…
The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
Ciro Pappalardo, George J. Bendo, Mederic Boquien +4
In recent years, significant growth in the amount of data available to astronomers has opened up the possibility to uncover fundamental correlations, linking the dust component of…
The differential energy distribution and the total integrated binding energy of dynamical models
Maarten Baes, Herwig Dejonghe
We revisit the differential energy distribution of steady-state dynamical models. It has been shown that the differential energy distribution of steady-state spherical models does…
Geometry effects on dust attenuation curves with different grain sources at high redshift
Yen-Hsing Lin, Hiroyuki Hirashita, Peter Camps +1
Dust has been detected in high-redshift () galaxies but its origin is still being debated. Dust production in high-redshift galaxies could be dominated by stellar production o…
First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
Aswin P. Vijayan, Stephen M. Wilkins, Christopher C. Lovell +6
Using the First Light And Reionisation Epoch Simulations (\textsc{Flares}) we explore the dust driven properties of massive high-redshift galaxies at . By post-processi…