Results 81 to 90 of about 1,565,970 (180)
The Impact of the Group Environment on the O vi Circumgalactic Medium
Abstract We present a study comparing O vi λλ1031, 1037 doublet absorption found toward group galaxy environments to that of isolated galaxies. The O vi absorption in the circumgalactic medium (CGM) of isolated galaxies has been studied previously by the “Multiphase Galaxy Halos” survey, where the kinematics and ...
Stephanie K. Pointon +5 more
openaire +5 more sources
CloudFlex: Modeling the Small-Scale Circumgalactic Medium
<p>CloudFlex is an open-source Python package for modeling the observational signatures associated with the small-scale structure of the circumgalactic medium.
Rubin, Kate +3 more
core +1 more source
Resolving Turbulence Drivers in Two Luminous Obscured Quasars with JWST/NIRSpec Integral Field Unit
In this Letter, we investigate the turbulence and energy injection in the extended nebulae surrounding two luminous obscured quasars, WISEA J100211.29+013706.7 ( z = 1.5933) and SDSS J165202.64+172852.3 ( z = 2.9489).
Mandy C. Chen +12 more
doaj +1 more source
Mapping the Circumgalactic Medium: Connecting Galaxies to their Environment
Thesis (Ph.D.)--University of Washington, 2022The work presented in this dissertation provides the groundwork for understanding key unresolved questions in the study of galaxy evolution: the circumgalactic medium (CGM) and the role of environment.
Wilde, Matthew
core
Abundance and temperature of the outer hot circumgalactic medium
Context. Despite their vital importance to understanding galaxy evolution and our own Galactic ecosystem, our knowledge of the physical properties of the hot X-ray emitting phase of the Milky Way is still inadequate.
X. Zheng +33 more
core +1 more source
Low-redshift fast radio bursts (FRBs) enable robust measurements of the host galaxy contribution to the dispersion measure (DM), offering valuable constraints on the circumgalactic medium (CGM) of FRB hosts.
Calvin Leung +23 more
doaj +1 more source
Turbulence driven by structure formation in the circumgalactic medium
The injection of turbulence in the circumgalactic medium at redshift z = 2 is investigated using the mesh-based hydrodynamic code ENZO and a sub-grid-scale (SGS) model for unresolved turbulence. Radiative cooling and heating by a uniform Ultraviolet (UV)
Viel M +7 more
core +1 more source
On the Origin of the 107 K Hot Emitting Gas in the Circumgalactic Medium of the Milky Way
The presence of the ≈10 ^6 K gas in the circumgalactic medium of the Milky Way (MW) has been well established. However, the location and the origin of the newly discovered hot gas at “supervirial (SV)” temperatures of ≈10 ^7 K have been puzzling.
Mukesh Singh Bisht +2 more
doaj +1 more source
Modern cosmology and galaxy formation rely on an understanding of how cosmic baryons are distributed, a significant portion of which exists in the diffuse gas confined to halos. Fast radio bursts (FRBs) are a promising probe of the Universe’s ionized gas.
Samuel McCarty +2 more
doaj +1 more source
Dual-disk galaxies and thermal states of circumgalactic medium
Disk galaxies often have dual-disk structures composed of thin disks and thick disks. Recent observations reveal that such duality is ubiquitous across broad galaxy mass and cosmic time.
Masafumi Noguchi
doaj +1 more source

