Results 131 to 140 of about 5,865 (191)

Galactic Cosmic Ray Interaction with the Perseus Giant Molecular Cloud Using Geant4 Monte Carlo Simulation

open access: yesUniverse
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

open access: yesThe Astrophysical Journal
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

open access: yesThe Astrophysical Journal
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

open access: yesThe Astrophysical Journal
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

Kilonovae. [PDF]

open access: yesLiving Rev Relativ, 2020
Metzger BD.
europepmc   +1 more source

Polarisation from Pulsar Wind Nebulae [PDF]

open access: yesProceedings of Polarimetry days in Rome: Crab status, theory and prospects — PoS(CRAB2008), 2009
Delia Volpi   +3 more
openaire   +1 more source

Spatial Variations and Breaks in the Optical–Near-infrared Spectra of the Pulsar and Pulsar Wind Nebula in Supernova Remnant 0540–69.3

open access: yesThe Astrophysical Journal
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]

open access: yesAstrophys J, 2019
Jóhannesson G   +2 more
europepmc   +1 more source

CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]

open access: yesAstrophys J, 2017
Wadiasingh Z   +4 more
europepmc   +1 more source

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