150 citations · 492 across the 7 of their papers we have counts for
7 papers
Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
Yannick M. Bahé, Joop Schaye, David J. Barnes +6
We investigate the disruption of group and cluster satellite galaxies with total mass (dark matter plus baryons) above 10^10 M_sun in the Hydrangea simulations, a suite of 24 high-…
Galaxies with monstrous black holes in galaxy cluster environments
Lieke A. C. van Son, Christopher Barber, Yannick M. Bahe +6
Massive early-type galaxies follow a tight relation between the mass of their central supermassive black hole () and their stellar mass (). The origin of…
Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
L. J. M. Davies, A. S. G. Robotham, C. del P. Lagos +16
Recently a number of studies have found a similarity between the passive fraction of central and satellite galaxies when controlled for both stellar and halo mass. These results su…
The environmental dependence of gas accretion onto galaxies: quenching satellites through starvation
Freeke van de Voort, Yannick M. Bahé, Richard G. Bower +4
Galaxies that have fallen into massive haloes may no longer be able to accrete gas from their surroundings, a process referred to as 'starvation' or 'strangulation' of satellites.…
SDSS IV MaNGA: Deep observations of extra-planar, diffuse ionized gas around late-type galaxies from stacked IFU spectra
A. Jones, G. Kauffmann, R. D'Souza +16
We have conducted a study of extra-planar diffuse ionized gas using the first year data from the MaNGA IFU survey. We have stacked spectra from 49 edge-on, late-type galaxies as a…
The origin of the enhanced metallicity of satellite galaxies
Yannick M. Bahe, Joop Schaye, Robert A. Crain +5
Observations of galaxies in the local Universe have shown that both the ionized gas and the stars of satellites are more metal-rich than of equally massive centrals. To gain insigh…