Results 111 to 120 of about 31,186 (206)
Statistical Properties of Cold Streams in Massive Star-forming Halos in TNG50
Cold, dense streams of gas are predicted to penetrate deeply into massive (≳10 ^12 M _⊙ ) halos at cosmic noon ( z ∼ 4–2), fueling galaxies to sustain high star formation rates.
Isabel Medlock +6 more
doaj +1 more source
The multiple coherence scales of C IV at cosmic noon
The spatial and kinematic structure of the circumgalactic medium remains poorly constrained observationally. We computed the clustering of C IV absorption systems at cosmic noon using quasar pairs.
Cortés-Muñoz H. +8 more
doaj +1 more source
Measurements of Cosmic Magnetism with LOFAR and SKA [PDF]
The origin of magnetic fields in stars, galaxies and clusters is an open problem in astrophysics. The next-generation radio telescopes <i>Low Frequency Array (LOFAR)</i> and <i>Square Kilometre Array (SKA)</i> will revolutionize ...
R. Beck
doaj
Considering light-matter interactions in Friedmann equations based on the conformal FLRW metric. [PDF]
Vavryčuk V.
europepmc +1 more source
Cascaded Gamma-Ray Emission Associated with the KM3NeT Ultrahigh-energy Event KM3-230213A
A neutrino-like event with an energy of ∼220 PeV was recently detected by the KM3NeT/ARCA telescope. If this neutrino comes from an astrophysical source or from the interaction of an ultrahigh-energy cosmic ray in the intergalactic medium, the ultrahigh ...
Ke Fang, Francis Halzen, Dan Hooper
doaj +1 more source
China's 'sky eye': exploring the universe by measuring faint cosmic radio signals. [PDF]
Zhao W.
europepmc +1 more source
Time Delay of Fast Radio Burst Population with Respect to the Star Formation History
In spite of significant progress in the research of fast radio bursts (FRBs) in recent decades, their origin is still under extensive debate. Investigation of the population of FRBs can provide new insight into this interesting problem.
Hai-Nan Lin, Xin-Yi Li, Rui Zou
doaj +1 more source
A New Approach for Constraining Large-scale Temperature Fluctuations in the Intergalactic Medium
The reionization of helium is thought to occur at 2.5 ≲ z ≲ 4, marking the last phase transition and final global heating event of the intergalactic medium (IGM).
Saba Etezad-Razavi +2 more
doaj +1 more source
Bioinformation and Neutrino Communication. [PDF]
Shapshak P.
europepmc +1 more source

