Results 71 to 80 of about 32,240 (255)

Predator's Prey: Reframing indigenous representation and Hollywood franchise cinema in the age of SVOD

open access: yesThe Journal of Popular Culture, Volume 57, Issue 3, Page 175-188, June 2024.
Abstract Hulu's Prey (2022), the fifth installment of the Predator franchise, is set in 1719 and features a Comanche female protagonist. The setting is unlike the 1987 Predator and its sequels, with their hardbody machismo and conservative politics. We argue that Prey is a small but significant step in Hollywood, but its inclusivity comes at a price ...
César Albarrán‐Torres, Andrew Lynch
wiley   +1 more source

Possible Contamination of the Intergalactic Medium Damping Wing in ULAS J1342+0928 by Proximate Damped Lyα Absorption

open access: yesThe Astrophysical Journal Letters
The red damping wing from neutral hydrogen in the intergalactic medium is a key predicted signature of ongoing reionization. One potential contaminant of the intergalactic damping wing signal is dense gas associated with foreground galaxies, which can ...
Frederick B. Davies   +3 more
doaj   +1 more source

Strategy to Explore Magnetized Cosmic Web with Forthcoming Large Surveys of Rotation Measure

open access: yesGalaxies, 2018
The warm-hot intergalactic medium (WHIM) is a candidate for the missing baryons in the Universe. If the WHIM is permeated with the intergalactic magnetic field (IGMF), the Faraday rotation measure (RM) of the WHIM is imprinted in linearly-polarized ...
Takuya Akahori
doaj   +1 more source

Evidence for strong extragalactic magnetic fields from Fermi observations of TeV blazars

open access: yes, 2010
Magnetic fields in galaxies are produced via the amplification of seed magnetic fields of unknown nature. The seed fields, which might exist in their initial form in the intergalactic medium, were never detected. We report a lower bound $B\ge 3\times 10^{
A. Neronov   +6 more
core   +1 more source

Gamma-Ray Background from Structure Formation in the Intergalactic Medium [PDF]

open access: yes, 2000
The universe is filled with a diffuse and isotropic extragalactic background of gamma-ray radiation, containing roughly equal energy flux per decade in photon energy between 3 MeV-100 GeV.
Abraham Loeb   +26 more
core   +2 more sources

The Cosmic Ultraviolet Baryon Survey (CUBS). IX. The Enriched Circumgalactic and Intergalactic Medium Around Star-forming Field Dwarf Galaxies Traced by O vi Absorption

open access: yesThe Astrophysical Journal
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

Simulating the Enrichment of Fossil Radio Electrons by Multiple Radio Galaxies

open access: yesGalaxies, 2023
We simulate the evolution of relativistic electrons injected into the intracluster medium by five radio galaxies. We study the spatial transport and the emission properties of the injected radio plasma over a ∼5 Gyr period, and the sequence of cooling ...
Franco Vazza   +3 more
doaj   +1 more source

Cosmic neutrino flux and spin flavor oscillations in intergalactic medium [PDF]

open access: green, 2022
Ashutosh Kumar Alok   +2 more
openalex   +1 more source

Intergalactic Medium Rotation Measure of Primordial Magnetic Fields

open access: yesThe Astrophysical Journal
The Faraday rotation effect, quantified by the rotation measure (RM), is a powerful probe of the large-scale magnetization of the Universe—tracing magnetic fields not only on galaxy and galaxy cluster scales but also in the intergalactic medium (IGM ...
Salome Mtchedlidze   +7 more
doaj   +1 more source

Galactic Winds in the Intergalactic Medium

open access: yesThe Astrophysical Journal, 2002
We have performed hydrodynamical simulations to investigate the effects of galactic winds on the high-redshift (z=3) universe. Strong winds suppress the formation of low-mass galaxies significantly, and the metals carried by them produce C IV absorption lines with properties in reasonable agreement with observations. The winds have little effect on the
THEUNS T   +5 more
openaire   +3 more sources

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