40 citations · 40 across the 1 of their papers we have counts for
5 papers
Mixing matters
Douglas Rennehan
All hydrodynamical simulations of turbulent astrophysical phenomena require sub-grid scale models to properly treat energy dissipation and metal mixing. We present the first implem…
Is there enough star formation in simulated protoclusters?
Seunghwan Lim, Douglas Scott, Arif Babul +5
As progenitors of the most massive objects, protoclusters are key to tracing the evolution and star-formation history of the Universe, and are responsible for per c…
Rapid early coeval star formation and assembly of the most massive galaxies in the universe
Douglas Rennehan, Arif Babul, Christopher C. Hayward +3
The current consensus on the formation and evolution of the brightest cluster galaxies is that their stellar mass forms early () in separate galaxies that then eventua…
Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
Douglas Rennehan, Arif Babul, Philip F. Hopkins +2
Modelling the turbulent diffusion of thermal energy, momentum, and metals is required in all galaxy evolution simulations due to the ubiquity of turbulence in galactic environments…
A massive core for a cluster of galaxies at a redshift of 4.3
T. B. Miller, S. C. Chapman, M. Aravena +35
Massive galaxy clusters are now found as early as 3 billion years after the Big Bang, containing stars that formed at even earlier epochs. The high-redshift progenitors of these ga…