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Highly ionized gas on galaxy scales: mapping the interacting Seyfert galaxy LEDA 135736
J. Gerssen, D. J. Wilman, L. Christensen +2
We have used the VIMOS IFU to map the properties of the Seyfert 1.9 galaxy LEDA 135736. These maps reveal a number of interesting features including: an Extended Narrow Line Region…
The flip-side of galaxy formation: A combined model of Galaxy Formation and Cluster Heating
Richard G. Bower, Ian G. McCarthy, Andrew J. Benson
Only ~10% of baryons in the universe are in the form of stars, yet most models of luminous structure formation have concentrated on the properties of the luminous stellar matter. I…
The Colours of Satellite Galaxies in Groups and Clusters
Andreea S. Font, Richard G. Bower, Ian G. McCarthy +6
Current models of galaxy formation predict satellite galaxies in groups and clusters that are redder than observed. We investigate the effect on the colours of satellite galaxies p…
Evolution in the Disks and Bulges of Group Galaxies since z=0.4
Sean L. McGee, Michael L. Balogh, Robert D. E. Henderson +4
We present quantitative morphology measurements of a sample of optically selected group galaxies at 0.3 < z < 0.55 using the Hubble Space Telescope (HST) Advanced Camera for Survey…
The clustering of the first galaxy halos
Darren S. Reed, Richard Bower, Carlos S. Frenk +2
We explore the clustering properties of high redshift dark matter halos, focusing on halos massive enough to host early generations of stars or galaxies at redshift 10 and greater.…
Unveiling the Important Role of Groups in the Evolution of Massive Galaxies: Insights from an Infrared Passive Sequence at Intermediate Redshift
D. J. Wilman, D. Pierini, K. Tyler +6
The most massive galaxies in the Universe are also the oldest. To overturn this apparent contradiction with hierarchical growth models, we focus on the group scale haloes which hos…