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Simulating Star Formation and Feedback in Galactic Disk Models
Elizabeth J. Tasker, Greg L. Bryan
We use a high-resolution grid-based hydrodynamics method to simulate the multi-phase interstellar medium in a Milky Way-size quiescent disk galaxy. The models are global and three-…
Simulations of thermally broadened HI Lya absorption arising in the warm-hot intergalactic medium
P. Richter, T. Fang, G. L. Bryan
Recent far-ultraviolet (FUV) absorption line measurements of low-redshift quasars have unveiled a population of intervening broad HI Lya absorbers (BLAs) with large Doppler paramet…
An X-ray Galaxy Cluster Survey for Investigations of Dark Energy
Z. Haiman, S. Allen, N. Bahcall +34
The amount and nature of dark energy (DE) can be tightly constrained by measuring the spatial correlation features and evolution of a sample of ~ 100,000 galaxy clusters over the r…
Cooling and Clusters: When Is Heating Needed?
Greg L. Bryan, G. Mark Voit
There are (at least) two unsolved problems concerning the current state of the thermal gas in clusters of galaxies. The first is identifying the source of the heating which offsets…