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Role of Cosmic Rays in the Circumgalactic Medium
Munier Salem, Greg L. Bryan, Lauren Corlies
We explore the impact of cosmic rays (CRs) on cosmological adaptive-mesh refinement simulations of a forming 10^12 Msolar halo, focusing on the circumgalactic medium (CGM), and its…
Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
Andrew Emerick, Greg Bryan, Mary E. Putman
Understanding gas flows into and out of the most massive dark matter structures in our Universe, galaxy clusters, is fundamental to understanding their evolution. Gas in clusters i…
Ram Pressure Stripping of the Large Magellanic Cloud's Disk as a Probe of the Milky Way's Circumgalactic Medium
Munier Salem, Gurtina Besla, Greg Bryan +3
Recent observations have constrained the orbit and structure of the Large Magellanic Cloud (LMC), implying a well-constrained pericentric passage about the Milky Way (MW) ~ 50 Myr…
Supernova Feedback and the Hot Gas Filling Fraction of the Interstellar Medium
Miao Li, Jeremiah P. Ostriker, Renyue Cen +2
Supernovae (SN), the most energetic stellar feedback mechanism, are crucial for regulating the interstellar medium (ISM) and launching galactic winds. We explore how supernova remn…
Precipitation-Regulated Star Formation in Galaxies
G. Mark Voit, Greg L. Bryan, Brian W. O'Shea +1
Galaxy growth depends critically on the interplay between radiative cooling of cosmic gas and the resulting energetic feedback that cooling triggers. This interplay has proven exce…
Limits on Population III star formation in minihaloes implied by Planck
Eli Visbal, Zoltan Haiman, Greg L. Bryan
Recently, Planck measured a value of the cosmic microwave background (CMB) optical depth due to electron scattering of . Here we show that this low value leaves…