We employ numerical simulations of galaxy mergers to explore the effect of galaxy mass
ratio on merger-driven starbursts. Our numerical simulations include radiative cooling of gas …

In this paper, we study the properties of pseudobulges (bulges that appear similar to disk
galaxies) and classical bulges (bulges which appear similar to E-type galaxies) in bulge …

Context. Bars are very common in the centre of the disc galaxies, and they drive the
evolution of their structure. The state-of-the-art imaging and redshift surveys of galaxies …

We present a catalog of visual-like H-band morphologies of∼ 50.000 galaxies (H f160w<
24.5) in the 5 CANDELS fields (GOODS-N, GOODS-S, UDS, EGS, and COSMOS) …

We use the bulge Sérsic index n and bulge-to-total mass ratio (B/T) to explore the
fundamental question of how bulges form. We perform two-dimensional bulge–disk–bar …

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 investigate scaling relations of bulges using bulge–disk decompositions at 3.6 μm and
present bulge classifications for 173 E-Sd galaxies within 20 Mpc. Pseudobulges and …

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 …

In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly
observed with the X-shooter spectrograph until 31/03/2017. In total, we have obtained …

Context. Historically, galaxy bulges were thought to be single-component objects at the
center of galaxies. However, this picture is now questioned since different bulge types with …