Results 61 to 70 of about 4,214,854 (199)
The Astrophysical Journal, 2023 Far-infrared polarized emission by means of magnetically aligned dust grains is an excellent tracer of the magnetic fields (B-fields) in the cold phase of the galactic outflows of starburst galaxies.
Enrique Lopez-Rodriguez
doaj +1 more source
Detection of extragalactic magnetic massive stars [PDF]
Astronomy & Astrophysicsodot $ leave behind neutron stars and black holes by the end of their evolution. The merging of binary compact remnant systems produces astrophysical transients detectable by gravitational wave observatories.
S. Hubrig +6 more
semanticscholar +1 more source
Extragalactic electromagnetic cascades and cascade gamma-ray emission in magnetic fields of various strength [PDF]
, 2023 We discuss the magnetic field influence on diffuse gamma-ray emission from extragalactic electromagnetic cascades initiated by ultra-high energy cosmic rays.
Uryson, A.
core +1 more source
Model of Super-Alfvénic MHD Turbulence and Statistics of Polarization
The Astrophysical JournalMHD turbulence driven at velocities higher than the Alfvén velocity, i.e., super-Alfvénic turbulence, is widely spread in astrophysical environments, including galaxy clusters and molecular clouds.
A. Lazarian, D. Pogosyan, Yue Hu
doaj +1 more source
Space Weather, Volume 24, Issue 8, August 2026.Abstract The period from 1 to 14 May 2024 was marked by some of the most intense solar activity of Solar Cycle 25, including multiple X‐class flares, fast coronal mass ejections (CMEs), and diverse solar radio emissions. We present observations from the Mexican e‐Callisto network (REC‐Mx), including long‐duration continuum emissions (CTMs), Type II ...
E. Aguilar‐Rodriguez +23 more
wiley +1 more source
Origin and Evolution of Large-scale Magnetic Fields [PDF]
, 2015 Magnetic elds are ubiquitous at all scales in the Universe and have been observed in galaxies and clusters of galaxies via observations of di use radio emission and Faraday Rotation Measures.
Barnes, DJ
core
The investigation of quasi-separatrix layers in solar magnetic fields [PDF]
, 2011 The structure of the magnetic field is often an important factor in many energetic processes in the solar corona. To determine the topology of the magnetic field features such as null points, separatrix surfaces, and separators must be found.
Restante, Anna Lisa
core +2 more sources
On the Detection of Low‐Frequency Planetary Radio Emission With an Orbiting Interferometer
Radio Science, Volume 61, Issue 6, June 2026.Abstract The magnetized planets of the outer Solar System produce kilometric radio emissions at very low frequencies (<1 ${< } 1\,$MHz). They reveal the planetary magnetic dynamics and their interaction with the solar wind. Those radio emissions can also serve as a proxy for interplanetary space weather monitoring.
E. Rouillé +4 more
wiley +1 more source
New Insights in Extragalactic Magnetic Fields
, 2019 Book collecting all the conference proceedings of Focus Meeting 8 "New Insights in Extragalactic Magnetic Fields" at the XXXth IAU General Assembly in Vienna ...
Feretti, Luigina +2 more
core +1 more source
CTAO sensitivity to axion-like particles [PDF]
EPJ Web of ConferencesAxion-like particles (ALPs) are a common feature in several extensions of the StandardModel, arising, for example, as a solution to the strong CP problem in quantum chromodynamics, or as a prediction of string theories.
Schiavone Francesco +2 more
doaj +1 more source