From a sample of 72 galaxies with reliable supermassive black hole masses M bh, we
derive the M bh–(host spheroid luminosity, L) relation for (1) the subsample of 24 core …

Photometric scaling relations are studied for S0 galaxies and compared with those obtained
for spirals. New two-dimensional multi-component decompositions are presented for 122 …

We have modelled the light distribution in 10 095 galaxies from the Millennium Galaxy
Catalogue (MGC), providing publicly available structural catalogues for a large …

From a quantitative analysis of 413 Virgo Cluster early-type dwarf galaxies (dEs) with SDSS
imaging data, we find that the dE class can be divided into multiple subpopulations that differ …

We present a systematic search for disk features in 476 Virgo Cluster early-type dwarf (dE)
galaxies. This is the first such study of an almost-complete, statistically significant dE sample …

Context. A variety of formation scenarios have been proposed to explain the diversity of
properties observed in bulges. Studying their intrinsic shape can help to constrain the …

We conduct a comprehensive numerical study of the orbital dependence of harassment on
early-type dwarfs consisting of 168 different orbits within a realistic, Virgo-like cluster …

The formation ofearly‐type dwarf (dE) galaxies, the most numerous objects in clusters, is
believed tobe closely connected to the physical processes that drive galaxy cluster …

A CATALOG OF VISUALLY CLASSIFIED GALAXIES IN THE LOCAL (z ∼ 0.01) UNIVERSE -
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The fraction of star-forming to quiescent dwarf galaxies varies from almost infinity in the field
to zero in the centers of rich galaxy clusters. What is causing this pronounced morphology …