Journal: Monthly Notices of the Royal Astronomical Society
Publication
Binary stars in the Galactic thick disc
The combination of asteroseismologically measured masses with abundances from detailed analyses of stellar atmospheres challenges our fundamental knowledge of...
BIRTH of the COSMOS field: primordial and evolved density reconstructions during cosmic high noon
This work presents the first comprehensive study of structure formation at the peak epoch of cosmic star formation over 1.4 ≤ z ≤ 3.6 in the Cosmic Evolution...
BIRTH of the COSMOS field: primordial and evolved density reconstructions during cosmic high noon
This work presents the first comprehensive study of structure formation at the peak epoch of cosmic star formation over 1.4 ≤ z ≤ 3.6 in the Cosmic Evolution...
Black hole mass and spin measurements through the relativistic precession model: XTE J1859+226
The X-ray light curves of accreting black holes and neutron stars in binary systems show various types of quasi-periodic oscillations (QPOs), the origin of...
Black hole masses of tidal disruption event host galaxies II
We present new medium resolution, optical long-slit spectra of a sample of six ultraviolet (UV)/optical and 17 X-ray-selected tidal disruption event candidate...
We present integral field spectroscopic observations of the central region of the active galaxy NGC 4258 obtained with the fibre IFU system INTEGRAL. We have...
Blue not brown: UKIRT Infrared Deep Sky Survey T dwarfs with suppressed K-band flux
We have used blue near-infrared colours to select a group of 12 spectroscopically confirmed United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey...
Blue straggler star (BSS) candidates have been observed in all old dwarf spheroidal galaxies (dSphs), however whether or not they are authentic BSSs or young...
Blue straggler stars in dwarf spheroidal galaxies - II. Sculptor and Fornax
The existence of blue straggler stars (BSSs) in dwarf spheroidal galaxies (dSphs) is still an open question. In fact, many BSS candidates have been observed in...