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Theoretical challenges in galaxy formation
Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …
evolution. Over the decades the field has made significant progress. It is now possible to …
The role of magnetic field in molecular cloud formation and evolution
We review the role that magnetic field may have on the formation and evolution of molecular
clouds. After a brief presentation and main assumptions leading to ideal MHD equations …
clouds. After a brief presentation and main assumptions leading to ideal MHD equations …
Pressure-regulated, feedback-modulated star formation in disk galaxies
The star formation rate (SFR) in galactic disks depends on both the quantity of the available
interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …
interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …
Cloud-scale molecular gas properties in 15 nearby galaxies
We measure the velocity dispersion, σ, and surface density, Σ, of the molecular gas in
nearby galaxies from CO spectral line cubes with spatial resolution 45–120 pc, matched to …
nearby galaxies from CO spectral line cubes with spatial resolution 45–120 pc, matched to …
A unified model for galactic discs: star formation, turbulence driving, and mass transport
We introduce a new model for the structure and evolution of the gas in galactic discs. In the
model the gas is in vertical pressure and energy balance. Star formation feedback injects …
model the gas is in vertical pressure and energy balance. Star formation feedback injects …
But what about...: cosmic rays, magnetic fields, conduction, and viscosity in galaxy formation
We present and study a large suite of high-resolution cosmological zoom-in simulations,
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …
Dynamical equilibrium in the molecular ISM in 28 nearby star-forming galaxies
We compare the observed turbulent pressure in molecular gas, P turb, to the required
pressure for the interstellar gas to stay in equilibrium in the gravitational potential of a …
pressure for the interstellar gas to stay in equilibrium in the gravitational potential of a …
Three-phase interstellar medium in galaxies resolving evolution with star formation and supernova feedback (TIGRESS): algorithms, fiducial model, and convergence
We introduce TIGRESS, a novel framework for multi-physics numerical simulations of the
star-forming interstellar medium (ISM) implemented in the Athena MHD code. The …
star-forming interstellar medium (ISM) implemented in the Athena MHD code. The …
Numerical simulations of multiphase winds and fountains from star-forming galactic disks. I. Solar neighborhood TIGRESS model
Gas blown away from galactic disks by supernova (SN) feedback plays a key role in galaxy
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
FORGE'd in FIRE: Resolving the End of Star Formation and Structure of AGN Accretion Disks from Cosmological Initial Conditions
It has recently become possible to zoom-in from cosmological to sub-pc scales in galaxy
simulations to follow accretion onto supermassive black holes (SMBHs). However, at some …
simulations to follow accretion onto supermassive black holes (SMBHs). However, at some …