830 citations · 4.7k across the 78 of their papers we have counts for
78 papers
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…
The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe
Viviana Casasola, Simone Bianchi, Pieter De Vis +18
The purpose of this work is the characterization of the main scaling relations between all the ISM components (dust, atomic/molecular/total gas), gas-phase metallicity, and other g…
Observational Properties of Field UDGs: Colours and Number Densities
Daniel J. Prole, Remco F. J. van der Burg, Michael Hilker +1
While much of the focus around Ultra-Diffuse Galaxies (UDGs) has been given to those in galaxy groups and clusters, relatively little is known about them in less-dense environments…
The First Maps of -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
Christopher J. R. Clark, Pieter De Vis, Maarten Baes +17
The dust mass absorption coefficient, , is the conversion function used to infer physical dust masses from observations of dust emission. However, it is notoriously poorly c…
The Widefield Arecibo Virgo Extragalactic Survey I: New structures in the ALFALFA Virgo 7 cloud complex and an extended tail on NGC 4522
Robert F. Minchin, Rhys Taylor, Joachim Köppen +3
We are carrying out a sensitive blind survey for neutral hydrogen (HI) in the Virgo cluster and report here on the first 5° x 1° area covered, which includes two optically-dark gas…
Observational Properties of Ultra-Diffuse Galaxies in the Field: Field-UDGs are Predominantly Blue and Starforming
Daniel J. Prole, Remco F. J. van der Burg, Michael Hilker +1
While we have learned much about Ultra-Diffuse Galaxies (UDGs) in groups and clusters, relatively little is known about them in less-dense environments. More isolated UDGs are impo…