Results 81 to 90 of about 1,993,973 (222)
Utilizing the Dispersion Measure of Fast Radio Bursts to Probe the Intergalactic Medium Turbulence
The Astrophysical JournalExtragalactic fast radio bursts (FRBs) have emerged as powerful probes of turbulence within the intergalactic medium (IGM), a phenomenon that plays a crucial role in various cosmological and astrophysical processes. In this study, we employ the structure
Rui-Nan Li +5 more
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The X-ray flux from the warm-hot intergalactic medium
, 2007 In the past years significant efforts have been focused on describing the evolution and structure of the Universe. One of the big open questions in cosmology is "Where is the baryonic mass"?
Ursino, Eugenio
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Cosmological Blast Waves and the Intergalactic Medium [PDF]
The Astrophysical Journal, 1996 Winds from protogalactic starbursts and quasars can drive shocks that heat, ionize, and enrich the intergalactic medium. The Sedov-Taylor solution for point-like explosions adequately describes these blastwaves early in their development, but as the time since the explosion ($t - t_1$) approaches the age of the universe ($t$), cosmological effects ...
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Chronicling the Reionization History at 6 ≲ z ≲ 7 with Emergent Quasar Damping Wings
The Astrophysical JournalThe spectra of high-redshift ( z ≳ 6) quasars contain valuable information on the progression of the Epoch of Reionization. At redshifts z < 6, the observed Lyman-series forest shows that the intergalactic medium is nearly ionized, while at z > 7 the ...
Dominika Ďurovčíková +8 more
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The intergalactic medium (IGM) comprises all the matter that lies between galaxies. Hosting the vast majority ($\gtrsim 90\%$) of the baryons in the Universe, the IGM is a critical reservoir and probe for cosmology and astrophysics, providing insights into large-scale structure formation and galaxy evolution.
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Dynamical evolution of high velocity clouds in the intergalactic medium
, 2002 $\ion{H}{i}$ observations of high-velocity clouds (HVCs) indicate, that they are interacting with their ambient medium. Even clouds located in the very outer Galactic halo or the intergalactic space seem to interact with their ambient medium.
G. T. Birk, C. Konz, C. Brüns
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Bird's-eye View of Molecular Gas across Stephan's Quintet Galaxy Group and Intragroup Medium
The Astrophysical JournalWe present the large-scale distribution and kinematics of cold molecular gas across the compact galaxy group Stephan’s Quintet, based on CO(2–1) observations performed with the Atacama Compact Array (ACA) and CO(1–0) data from the Combined Array for ...
B. H. C. Emonts +17 more
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Probing the thermal history of the Intergalactic Medium with
, 2007 The Doppler parameter distribution of Lyff absorption is calculated for a set of different reionization histories. The differences in temperature between different reionization histories are as large as a factor three to four depending on the spectrum of
Martin G. Haehnelt +2 more
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, 2023 <p>The uploaded files can be used to reproduce the dataset and figures in the paper<strong> Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight</strong> ...
Štofanová, Lýdia
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The Astrophysical JournalX-ray photons substantially affect the thermal and ionization states of the intergalactic medium during the epoch of reionization (EoR), thereby significantly influencing the 21 cm line observables, such as its sky-averaged (global) brightness ...
S. Mobina Hosseini, Bahareh S. Salmasi
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