Results 131 to 140 of about 5,865 (191)
Galactic cosmic rays (GCRs), composed of protons and atomic nuclei, are accelerated in sources such as supernova remnants and pulsar wind nebulae, reaching energies up to the PeV range.
Luan Torres, Luiz Augusto Stuani Pereira
doaj +1 more source
Analysis of Crab X-Ray Polarization Using Deeper Imaging X-Ray Polarimetry Explorer Observations
We present Crab X-ray polarization measurements using Imaging X-Ray Polarimetry Explorer (IXPE) data with a total exposure of 300 ks, three times more than the initial 2022 discovery paper.
Josephine Wong +100 more
doaj +1 more source
Potential Contribution of Young Pulsar Wind Nebulae to Galactic High-energy Neutrino Emission
Pulsar wind nebulae (PWNe), especially the young ones, are among the most energetic astrophysical sources in the Galaxy. It is usually believed that the spin-down energy injected from the pulsars is converted into magnetic field and relativistic ...
Xuan-Han Liang +4 more
doaj +1 more source
Study of Magnetic Field and Turbulence in the TeV Halo around the Monogem Pulsar
Magnetic fields are ubiquitous in the interstellar medium, including extended objects such as supernova remnants and diffuse halos around pulsars. Its turbulent characteristics govern the diffusion of cosmic rays and the multiwavelength emission from ...
Sunil Malik, Ka Ho Yuen, Huirong Yan
doaj +1 more source
Signatures of Recent Cosmic-Ray Acceleration in the High-latitude Gamma-Ray Sky. [PDF]
Jóhannesson G, Porter TA.
europepmc +1 more source
Polarisation from Pulsar Wind Nebulae [PDF]
Delia Volpi +3 more
openaire +1 more source
The supernova remnant (SNR) 0540–69.3, twin of the Crab Nebula, offers an excellent opportunity to study the continuum emission from a young pulsar and pulsar wind nebula (PWN). We present observations taken with the Very Large Telescope instruments MUSE
L. Tenhu +6 more
doaj +1 more source
Cosmic-Ray Propagation in Light of the Recent Observation of Geminga. [PDF]
Jóhannesson G +2 more
europepmc +1 more source
CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]
Wadiasingh Z +4 more
europepmc +1 more source

