We present an analysis of V-band radial surface brightness μ(r) profiles for S0 galaxies in different environments using Hubble Space Telescope/Advanced Camera for Surveys imaging and data from the Space Telescope A901/2 Galaxy Evolution Survey. Using a large sample of ∼280 field and cluster S0s, we find that in both environments, ∼25 per cent have a pure exponential disc (type I) and ∼50 per cent exhibit an up-bending disc break (antitruncation, type III). However, we find hardly any (<5 per cent) down-bending disc breaks (truncations, type II) in our S0s and many cases (∼20 per cent) where no discernible exponential component was observed (i.e. general curvature). We also find no evidence for an environmental dependence on the disc scalel...
We analyse the dependence of the stellar disc flatness on the galaxy morphological type using 2D dec...
We provide a physical interpretation and explanation of the morphology-density relation for galaxies...
With the aim of understanding the effect of the environment on the star formation history and morpho...
We present an analysis of V ‐band radial surface brightness profiles for spiral galaxies from the f...
In this thesis, we explore the effect of the galaxy environment on the physical size and structure o...
We present an analysis of V-band radial surface brightness profiles for spiral galaxies from the fie...
We analyse a high-resolution, fully cosmological, hydrodynamical disc galaxy simulation, to study th...
We study the surface brightness profiles of disc galaxies in the 3.6 μm images from the Spitze...
Aims. Using a sample of 175 low-inclination galaxies from the S(4)G, we investigate the origins of u...
Using imaging data from the SDSS survey, we present the g' and r' radial stellar light distribution ...
Context. It has been recently found that the characteristic photometric parameters of anti-truncated...
Aims. The physics driving features such as breaks observed in galaxy surface brightness (SB) profile...
We re-investigate the dramatic rise in the S0 fraction, f_(S0), within clusters since z ~ 0.5. In pa...
Different processes have been proposed to explain the formation of S0s, including mergers, disc inst...
The individual star formation histories of bulges and discs of lenticular (S0) galaxies can provide ...
We analyse the dependence of the stellar disc flatness on the galaxy morphological type using 2D dec...
We provide a physical interpretation and explanation of the morphology-density relation for galaxies...
With the aim of understanding the effect of the environment on the star formation history and morpho...
We present an analysis of V ‐band radial surface brightness profiles for spiral galaxies from the f...
In this thesis, we explore the effect of the galaxy environment on the physical size and structure o...
We present an analysis of V-band radial surface brightness profiles for spiral galaxies from the fie...
We analyse a high-resolution, fully cosmological, hydrodynamical disc galaxy simulation, to study th...
We study the surface brightness profiles of disc galaxies in the 3.6 μm images from the Spitze...
Aims. Using a sample of 175 low-inclination galaxies from the S(4)G, we investigate the origins of u...
Using imaging data from the SDSS survey, we present the g' and r' radial stellar light distribution ...
Context. It has been recently found that the characteristic photometric parameters of anti-truncated...
Aims. The physics driving features such as breaks observed in galaxy surface brightness (SB) profile...
We re-investigate the dramatic rise in the S0 fraction, f_(S0), within clusters since z ~ 0.5. In pa...
Different processes have been proposed to explain the formation of S0s, including mergers, disc inst...
The individual star formation histories of bulges and discs of lenticular (S0) galaxies can provide ...
We analyse the dependence of the stellar disc flatness on the galaxy morphological type using 2D dec...
We provide a physical interpretation and explanation of the morphology-density relation for galaxies...
With the aim of understanding the effect of the environment on the star formation history and morpho...