Results 51 to 60 of about 1,565,970 (180)
THE CIRCUMGALACTIC MEDIUM OF THE MILKY WAY IS HALF HIDDEN [PDF]
We assess the fraction of the Milky Way's circumgalactic medium (CGM) eluding detection due to its velocity being similar to gas in the disk. This is achieved using synthetic observations of the CGM in a simulated MW-mass galaxy that shows similar CGM kinematics to the MW and external L$\sim$L$_*$ galaxies.
Y. Zheng +3 more
openaire +2 more sources
The physical nature of circumgalactic medium absorbers in
ABSTRACT We study the nature of the low-redshift circumgalactic medium (CGM) in the Simba cosmological simulations as traced by ultraviolet absorption lines around galaxies in bins of stellar mass ($\mbox{$M_\star $}\, > 10^{10}{\rm M}_\odot$) for star-forming, green valley and quenched galaxies at impact parameters r⊥ ≤ 1.25r200.
Sarah Appleby +4 more
openaire +4 more sources
The imprint of dark subhaloes on the circumgalactic medium [PDF]
ABSTRACT The standard model of cosmology, the Λ cold dark matter (ΛCDM) model, robustly predicts the existence of a multitude of dark matter ‘subhaloes’ around galaxies like the Milky Way. A wide variety of observations have been proposed to look for the gravitational effects such subhaloes would induce in observable matter.
Ian G McCarthy, Andreea S Font
openaire +2 more sources
We investigate the coevolution of the angular momentum of Milky Way–like galaxies, their circumgalactic gas, and their dark matter halos using zoom-in simulations from the Figuring Out Gas and Galaxies in Enzo suite.
Raymond C. Simons +12 more
doaj +1 more source
DUST IN THE CIRCUMGALACTIC MEDIUM OF LOW-REDSHIFT GALAXIES
Using spectroscopically selected galaxies from the Sloan Digital Sky Survey we present a detection of reddening effects from the circumgalactic medium of galaxies which we attribute to an extended distribution of dust.
Menard, Brice +2 more
core +1 more source
Ceci n’est pas une Couche de Mélange: The Meaning of Resolved Turbulent Radiative Mixing
Turbulent radiative mixing layers (TRMLs) are of fundamental importance to the transport of energy and momentum in multiphase, astrophysical fluids. We use measurements of the microscopic and macroscopic properties of these layers in high-resolution ...
Lachlan Lancaster +3 more
doaj +1 more source
This is a pre-print of a chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor S.
Chen, Hsiao-Wen, Zahedy, Fakhri S.
openaire +2 more sources
The Origin of Da Scaling: Suppressed Cooling in Fast-cooling Mixing Layers
In numerical experiments simulating turbulent radiative mixing layers (TRMLs), it is observed that as the cooling time in the mixed gas, t _cool , becomes very short compared to the dynamical time of the turbulence, t _eddy / t _cool ≫ 1, there is a ...
Lachlan Lancaster +3 more
doaj +1 more source
On the Origin of High-velocity Clouds in the Galaxy
The origin of our Galaxy’s high-velocity clouds (HVCs) remains a mystery after many decades of effort. In this paper, we use the TNG50 simulation of the IllustrisTNG project to identify cool, dense clouds that match observations of Galactic H i HVCs.
Scott Lucchini +3 more
doaj +1 more source
To understand how massive galaxies at high z coevolve with enormous reservoirs of halo gas, it is essential to study the coldest phase of the circumgalactic medium (CGM), which directly relates to stellar growth.
Jianrui Li +12 more
doaj +1 more source

