Results 81 to 90 of about 1,770 (180)
Understanding the thermodynamic properties of the circumgalactic medium (CGM) is key to uncovering the baryon cycle in galaxies. Here, we present spatial and kinematic relationships between Mg ii and O vi , as representatives for low- and high-ion ...
Mackenzie Ticoras +11 more
doaj +1 more source
Characterizing the Circumgalactic Medium in Emission [PDF]
In this thesis I focus on understanding the physical properties of extended Lyman-alpha emitting gas at high redshift, from the circumgalactic medium (CGM) and intergalactic medium (IGM). First, I investigate the physics of giant, luminous Lyman-alpha nebulae known as Lyman alpha blobs (LABs).
openaire +2 more sources
The shallow potential wells of star-forming dwarf galaxies make their surrounding circumgalactic and intergalactic medium (CGM/IGM) sensitive laboratories for studying the inflows and outflows thought to regulate galaxy evolution.
Nishant Mishra +15 more
doaj +1 more source
Impacts of the Metagalactic Ultraviolet Background on Circumgalactic Medium Absorption Systems
Among the many different pieces of physics that go into simulations of the circumgalactic medium (CGM), the metagalactic ultraviolet background (UVB) plays a significant role in determining the ionization state of different metal species.
Elias Taira +7 more
doaj +1 more source
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
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
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
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
Detection of diffuse HI emission in the circumgalactic medium of NGC891 and NGC4565 -- II
We probe the neutral circumgalactic medium (CGM) along the major axes of NGC891 and NGC4565 in 21-cm emission out to $\gtrsim 100$kpc using the Green Bank Telescope (GBT), extending our previous minor axes observations.
Pisano, D. J. +8 more
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