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Astronomy & Astrophysics, ISSN 0004-6361, 03/2016, Volume 587
Thanks to deep UV observations with GALEX and Swift, diffuse UV haloes have recently been discovered around galaxies. Based on UV-optical colours, it has been... 
Galactic halos | Cosmic dust | Galaxies | Spectral energy distribution | Disks | Radiative transfer | Infrared signatures | Diffusion
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2019, Volume 489, Issue 4, pp. 5256 - 5283
ABSTRACT The dust mass absorption coefficient, κd is the conversion function used to infer physical dust masses from observations of dust emission. However, it... 
Sciences of the Universe | Astrophysics
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 08/2016, Volume 592
We investigate the dust energy balance for the edge-on galaxy IC2531, one of the seven galaxies in the HEROES sample. We perform a state-of-the-art radiative... 
Dust | Parameters | Wavelengths | Galaxies | Astronomical models | Mathematical models | Radiative transfer | Modelling
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 02/2020, Volume 492, Issue 1, pp. 195 - 209
We present a CO(3-2) survey of selected regions in the M31 disc as part of the JCMT large programme, HARP and SCUBA-2 High-Resolution Terahertz Andromeda... 
NEARBY GALAXIES | FORMATION LAW | INNER DISK | J=3-2 SURVEY | DENSITY | DUST | TEMPERATURE | ISM: molecules | galaxies: ISM | CO EMISSION | ASTRONOMY & ASTROPHYSICS | MASSIVE MOLECULAR CLOUDS | galaxies: individual (M 31) | GAS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 03/2016, Volume 587, p. A86
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2016, Volume 462, Issue 1, pp. 331 - 331
In most studies of dust in galaxies, dust is only detected from its emission to approximately the optical radius of the galaxy. By combining the signal of 110... 
Quasars | Dust | Cosmic dust | Galaxies | Symbols | Disks | Constants | Density
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2015, Volume 451, Issue 2, pp. 1728 - 1728
Interstellar dust in galaxies can be traced either through its extinction effects on the star light or through its thermal emission at infrared wavelengths.... 
Dust | Balancing | Galaxies | Astronomical models | Mathematical models | Radiative transfer | Spiral galaxies | Fluxes
Journal Article