Results 121 to 130 of about 878 (215)
Potential Contribution of Young Pulsar Wind Nebulae to Galactic High-energy Neutrino Emission
The Astrophysical JournalPulsar 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
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Study of Magnetic Field and Turbulence in the TeV Halo around the Monogem Pulsar
The Astrophysical JournalMagnetic 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
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Multiband emission from pulsar wind nebulae: a possible injection spectrum [PDF]
, 2010 Jun Fang, Li Zhang
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The Astrophysical JournalThe gamma-ray halo around Geminga indicates significant suppression of cosmic-ray diffusion. One possible explanation for this phenomenon is the projection effect of slow diffusion perpendicular to the mean magnetic field (characterized by the diffusion ...
Junji Xia +3 more
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Deriving pulsar pair-production multiplicities from pulsar wind nebulae using H.E.S.S. and LHAASO observations [PDF]
S. Spencer, Alison Mitchell
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The effects of magnetic field, age and intrinsic luminosity on Crab-like pulsar wind nebulae [PDF]
, 2013 D. F. Torres +3 more
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Evidence of an Energetic Magnetar Powering 1LHAASO J0500+4454
The Astrophysical JournalWe investigate the origin of the unidentified, extended TeV source 1LHAASO J0500+4454, considering three possible origins: cosmic rays interacting with a molecular cloud (MC), particles accelerated in a currently undetected supernova remnant (SNR), and ...
J. A. J. Alford +3 more
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Signatures of Recent Cosmic-Ray Acceleration in the High-latitude Gamma-Ray Sky. [PDF]
Astrophys J, 2021 Jóhannesson G, Porter TA.
europepmc +1 more source
The Astrophysical JournalThe 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
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