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Physical properties of simulated galaxy populations at z=2 - II. Effects of cosmology, reionization and ISM physics
Marcel R. Haas, Joop Schaye, C. M. Booth +4
We use hydrodynamical simulations from the OWLS project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on the assumed star formation l…
Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN
Marcel R. Haas, Joop Schaye, C. M. Booth +4
We use hydrodynamical simulations from the OWLS project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on metal-line cooling and feedb…
Ubiquitous seeding of supermassive black holes by direct collapse
Bhaskar Agarwal, Sadegh Khochfar, Jarrett L. Johnson +3
We study for the first time the environment of massive black hole (BH) seeds (~10^4-5 Msun) formed via the direct collapse of pristine gas clouds in massive haloes (>10^7 Msun) at…
Simulating galactic outflows with thermal supernova feedback
Claudio Dalla Vecchia, Joop Schaye
Cosmological simulations make use of sub-grid recipes for the implementation of galactic winds driven by massive stars because direct injection of supernova energy in thermal form…