Journal: Monthly Notices of the Royal Astronomical Society
Publication
The magnetic SW Sextantis star RXJ1643.7+3402
We present time-resolved spectroscopy and circular spectropolarimetry of the SW Sex star RXJ1643.7+3402. We find significant polarization levels exhibiting a...
The MAGPI Survey: impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
We investigate the impact of environment on the internal mass distribution of galaxies using the Middle Ages Galaxy Properties with Integral field spectroscopy...
The MAGPI Survey: massive slow rotator population in place by z 0.3
We use the 'Middle Ages Galaxy Properties with Integral field spectroscopy' (MAGPI) survey to investigate whether galaxies have evolved in the distribution of...
The MAGPI survey: orbital distributions, intrinsic shapes, and mass profiles for MAGPI-like EAGLE galaxies using Schwarzschild dynamical models
Schwarzschild dynamical models are now regularly employed in large surveys of galaxies in the local and distant Universe to derive information on galaxies'...
The Mark-I helioseismic experiment - I. Measurements of the solar gravitational redshift (1976-2013)
The resonant scattering solar spectrophotometer `Mark-I', designed and build at the University of Birmingham (UK) and located at the Observatorio del Teide...
The mass and angular momentum distribution of simulated massive early-type galaxies to large radii
We study the dark and luminous mass distributions, circular velocity curves (CVCs), line-of-sight kinematics and angular momenta for a sample of 42 cosmological...
The mass and galaxy distribution around SZ-selected clusters
We present measurements of the radial profiles of the mass and galaxy number density around Sunyaev-Zel'dovich (SZ)-selected clusters using both weak lensing...
The mass of our Galaxy from satellite proper motions in the Gaia era
We use Gaia DR2 systemic proper motions of 45 satellite galaxies to constrain the mass of the Milky Way using the scale-free mass estimator of Watkins et al....
The mass of the black hole in GS 2000+25 (=QZ Vul).
The authors report the first infrared light curve of GS 2000+25. By modelling the brightness variations as ellipsoidal modulations of the secondary star, the...