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Astronomy & Astrophysics, ISSN 0004-6361, 10/2019, Volume 630, p. A113
We expand our previous analytical and numerical studies of the family of Sérsic models, which are routinely used to describe early-type galaxies and the bulges... 
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 06/2019, Volume 626, p. A110
The Sérsic or R1/m model has become the de facto standard model to describe the surface brightness profiles of early-type galaxies and the bulges of spiral... 
Journal Article
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
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2012, Volume 420, Issue 4, pp. 2756 - 2772
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 06/2019, Volume 626
The Sersic or R-1/m model has become the de facto standard model to describe the surface brightness profiles of early-type galaxies and the bulges of spiral... 
SPHERICAL GALAXIES | galaxies: photometry | DWARF ELLIPTIC GALAXIES | PARAMETERS | BULGES | ANISOTROPY | LIGHT PROFILES | FAMILY | galaxies: structure | SHAPE | MODELS | ASTRONOMY & ASTROPHYSICS | methods: analytical | galaxies: kinematics and dynamics | FUNDAMENTAL PLANE
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 3, pp. 2288 - 2302
Monthly Notices of the Royal Astronomical Society, 2016, 458, 2288-2302 The primary source of emission of active galactic nuclei (AGN), the accretion disk, is... 
Galaxies: Active | Radiative transfer | Galaxies: Nuclei | Galaxies: Seyfert | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2018, Volume 861, Issue 2, p. 80
Computer simulations of photon transport through an absorbing and/or scattering medium form an important research tool in astrophysics. Nearly all software... 
dust, extinction | methods: numerical | opacity | radiative transfer | DISC GALAXIES | REFLECTION NEBULAE | INTERSTELLAR DUST | CONFIDENCE-INTERVAL | TRANSPORT | SMALL GRAINS | ASTRONOMY & ASTROPHYSICS | TRANSFER SIMULATIONS | EMISSION | EXTINCTION | POLARIZATION | Physics - Instrumentation and Methods for Astrophysics
Journal Article
by Camps, P and Baes, M
Astronomy and Computing, ISSN 2213-1337, 03/2015, Volume 9, pp. 20 - 33
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, 2009, Volume 392, Issue 4, pp. 1503 - 1508
Cosmological simulations suggest that dark matter haloes are not spherical, but typically moderately to strongly triaxial systems. We investigate methods to... 
methods: analytical | dark matter | Dark matter |