Search Results - "Bryan, Greg L."
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Self-consistent Semianalytic Modeling of Feedback during Primordial Star Formation and Reionization
Published in The Astrophysical journal (01-07-2020)“…We present a new semianalytic model of the formation of the first stars. Our method takes dark matter halo merger trees (including three-dimensional spatial…”
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2
Direct collapse black hole formation from synchronized pairs of atomic cooling haloes
Published in Monthly notices of the Royal Astronomical Society (21-11-2014)“…High-redshift quasar observations imply that supermassive black holes (SMBHs) larger than ∼109 M⊙ formed before z ∼ 6. That such large SMBHs formed so early in…”
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3
The Critical Dark Matter Halo Mass for Population III Star Formation: Dependence on Lyman–Werner Radiation, Baryon-dark Matter Streaming Velocity, and Redshift
Published in The Astrophysical journal (01-08-2021)“…Abstract A critical dark matter halo mass ( M crit ) for Population III stars can be defined as the typical minimum halo mass that hosts sufficient cold-dense…”
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4
Star formation in ram pressure stripped galactic tails
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…We investigate the impact of star formation and feedback on ram pressure stripping using high-resolution adaptive mesh simulations, building on a previous…”
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Quantifying Supernovae-driven Multiphase Galactic Outflows
Published in The Astrophysical journal (01-06-2017)“…Galactic outflows are observed everywhere in star-forming disk galaxies and are critical for galaxy formation. Supernovae (SNe) play the key role in driving…”
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6
When and How Ram Pressure Stripping in Low-mass Satellite Galaxies Enhances Star Formation
Published in The Astrophysical journal (01-01-2024)“…Abstract We investigate how a satellite's star formation rate (SFR) and surviving gas respond to ram pressure stripping (RPS) in various environments. Using a…”
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Formation and evolution of young massive clusters in galaxy mergers: the SMUGGLE view
Published in Monthly notices of the Royal Astronomical Society (03-06-2022)“…ABSTRACT Galaxy mergers are known to host abundant young massive cluster (YMC) populations, whose formation mechanism is still not well-understood. Here, we…”
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The Impact of Galactic Winds on the Angular Momentum of Disk Galaxies in the Illustris Simulation
Published in The Astrophysical journal (20-05-2017)“…Observed galactic disks have specific angular momenta similar to expectations for typical dark matter halos in ΛCDM. Cosmological hydrodynamical simulations…”
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A Global Model for Circumgalactic and Cluster-core Precipitation
Published in The Astrophysical journal (10-08-2017)“…We provide an analytic framework for interpreting observations of multiphase circumgalactic gas that is heavily informed by recent numerical simulations of…”
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10
First Results from SMAUG: Characterization of Multiphase Galactic Outflows from a Suite of Local Star-forming Galactic Disk Simulations
Published in The Astrophysical journal (01-09-2020)“…Large-scale outflows in star-forming galaxies are observed to be ubiquitous and are a key aspect of theoretical modeling of galactic evolution, the focus of…”
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11
grackle: a chemistry and cooling library for astrophysics
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…We present the grackle chemistry and cooling library for astrophysical simulations and models. grackle provides a treatment of non-equilibrium primordial…”
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12
AGN Heating in Simulated Cool-core Clusters
Published in The Astrophysical journal (01-10-2017)“…We analyze heating and cooling processes in an idealized simulation of a cool-core cluster, where momentum-driven AGN feedback balances radiative cooling in a…”
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Characterizing mass, momentum, energy, and metal outflow rates of multiphase galactic winds in the FIRE-2 cosmological simulations
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT We characterize mass, momentum, energy, and metal outflow rates of multiphase galactic winds in a suite of FIRE-2 cosmological ‘zoom-in’ simulations…”
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14
It’s a Breeze: The Circumgalactic Medium of a Dwarf Galaxy Is Easy to Strip
Published in The Astrophysical journal (01-10-2024)“…Abstract The circumgalactic medium (CGM) of star-forming dwarf galaxies plays a key role in regulating the galactic baryonic cycle. We investigate how…”
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Evolution of Star Clusters within Galaxies Using Self-consistent Hybrid Hydro/N-body Simulations
Published in The Astrophysical journal (01-10-2024)“…Abstract We introduce a GPU-accelerated hybrid hydro/ N -body code ( Enzo-N ) designed to address the challenges of concurrently simulating star clusters and…”
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Taming the TuRMoiL: The Temperature Dependence of Turbulence in Cloud–Wind Interactions
Published in The Astrophysical journal (01-05-2024)“…Abstract Turbulent radiative mixing layers play an important role in many astrophysical contexts where cool (≲10 4 K) clouds interact with hot flows (e.g.,…”
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Constraints on hydrodynamical subgrid models from quasar absorption line studies of the simulated circumgalactic medium
Published in Monthly notices of the Royal Astronomical Society (11-04-2013)“…Cosmological hydrodynamical simulations of galaxy evolution are increasingly able to produce realistic galaxies, but the largest hurdle remaining is in…”
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18
Regulation of Star Formation by a Hot Circumgalactic Medium
Published in The Astrophysical journal (01-05-2023)“…Abstract Galactic outflows driven by supernovae (SNe) are thought to be a powerful regulator of a galaxy’s star-forming efficiency. Mass, energy, and metal…”
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The Anatomy of a Turbulent Radiative Mixing Layer: Insights from an Analytic Model with Turbulent Conduction and Viscosity
Published in The Astrophysical journal (01-06-2023)“…Abstract Turbulent radiative mixing layers (TRMLs) form at the interface of cold, dense gas and hot, diffuse gas in motion with each other. TRMLs are…”
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Which AGN jets quench star formation in massive galaxies?
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT Without additional heating, radiative cooling of the halo gas of massive galaxies (Milky Way-mass and above) produces cold gas or stars exceeding that…”
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