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Direct Detection of Black Hole-Driven Turbulence in the Centers of Galaxy Clusters
Yuan Li, Marie-Lou Gendron-Marsolais, Irina Zhuravleva +16
Supermassive black holes (SMBHs) are thought to provide energy that prevents catastrophic cooling in the centers of massive galaxies and galaxy clusters. However, it remains unclea…
Simple Yet Powerful: Hot Galactic Outflows Driven by Supernovae
Miao Li, Greg L. Bryan
Supernovae (SNe) drive multiphase galactic outflows, impacting galaxy formation; however, cosmological simulations mostly use \textit{ad hoc} feedback models for outflows, making o…
Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy
Andrew Emerick, Greg L. Bryan, Mordecai-Mark Mac Low
One-zone models constructed to match observed stellar abundance patterns have been used extensively to constrain the sites of nucleosynthesis with sophisticated libraries of stella…
The Impact of Type Ia Supernovae in Quiescent Galaxies: II. Energetics and Turbulence
Miao Li, Yuan Li, Greg L. Bryan +2
Type Ia supernovae (SNe Ia) provide unique and important feedback in quiescent galaxies, but their impact has been underappreciated. In this paper, we analyze a series of high-reso…
The Impact of Type Ia Supernovae in Quiescent Galaxies: I. Formation of the Multiphase Interstellar medium
Miao Li, Yuan Li, Greg L. Bryan +2
A cool phase of the interstellar medium has been observed in many giant elliptical galaxies, but its origin remains unclear. We propose that uneven heating from Type Ia supernovae…
Properties of the Simulated Circumgalactic Medium
Cassandra Lochhaas, Greg L. Bryan, Yuan Li +2
The circumgalactic medium (CGM) is closely linked to galaxy formation and evolution, but difficult to characterize observationally and typically poorly resolved in cosmological sim…