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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 …
Momentum injection by supernovae in the interstellar medium
Supernova (SN) explosions deposit prodigious energy and momentum in their
environments, with the former regulating multiphase thermal structure and the latter …
environments, with the former regulating multiphase thermal structure and the latter …
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 …
Raining on black holes and massive galaxies: the top-down multiphase condensation model
The plasma haloes filling massive galaxies, groups and clusters are shaped by active
galactic nucleus (AGN) heating and subsonic turbulence (σ v∼ 150 km s− 1), as probed by …
galactic nucleus (AGN) heating and subsonic turbulence (σ v∼ 150 km s− 1), as probed by …
Atomic and Ionized microstructures in the diffuse interstellar medium
S Stanimirović, EG Zweibel - Annual Review of Astronomy and …, 2018 - annualreviews.org
It has been known for half a century that the interstellar medium (ISM) of our Galaxy is
structured on scales as small as a few hundred kilometers, more than 10 orders of …
structured on scales as small as a few hundred kilometers, more than 10 orders of …
Formation of molecular clouds and global conditions for star formation
Giant molecular clouds (GMCs) are the primary reservoirs of cold, star-forming molecular
gas in the Milky Way and similar galaxies, and thus any understanding of star formation must …
gas in the Milky Way and similar galaxies, and thus any understanding of star formation must …
Star formation in disk galaxies. I. Formation and evolution of giant molecular clouds via gravitational instability and cloud collisions
We investigate the formation and evolution of giant molecular clouds (GMCs) in a Milky-Way-
like disk galaxy with a flat rotation curve. We perform a series of three-dimensional adaptive …
like disk galaxy with a flat rotation curve. We perform a series of three-dimensional adaptive …
Gas kinematics on giant molecular cloud scales in M51 with PAWS: cloud stabilization through dynamical pressure
We use the high spatial and spectral resolution of the PAWS CO (1–0) survey of the inner 9
kpc of the iconic spiral galaxy M51 to examine the effects of gas streaming motions on the …
kpc of the iconic spiral galaxy M51 to examine the effects of gas streaming motions on the …
The properties of the interstellar medium in disc galaxies with stellar feedback
We perform calculations of isolated disc galaxies to investigate how the properties of the
interstellar medium (ISM), the nature of molecular clouds and the global star formation rate …
interstellar medium (ISM), the nature of molecular clouds and the global star formation rate …
Regulation of star formation rates in multiphase galactic disks: numerical tests of the thermal/dynamical equilibrium model
We use vertically resolved numerical hydrodynamic simulations to study star formation and
the interstellar medium (ISM) in galactic disks. We focus on outer-disk regions where diffuse …
the interstellar medium (ISM) in galactic disks. We focus on outer-disk regions where diffuse …