Results 121 to 130 of about 6,070 (203)
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
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Mass-loading of bow shock pulsar wind nebulae [PDF]
Giovanni Morlino +2 more
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The 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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Pulsar Wind Nebulae as High Energy Gamma-Ray Emitters [PDF]
M. S. Roberts +2 more
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Diffusion and advection model for particle transport in young pulsar wind nebulae [PDF]
Xiaping Tang, Roger A. Chevalier
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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
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Signatures of Recent Cosmic-Ray Acceleration in the High-latitude Gamma-Ray Sky. [PDF]
Jóhannesson G, Porter TA.
europepmc +1 more source
Lessons from HAWC pulsar wind nebulae observations: The diffusion constant is not a constant; pulsars remain the likeliest sources of the anomalous positron fraction; cosmic rays are trapped for long periods of time in pockets of inefficient diffusion [PDF]
Stefano Profumo +3 more
openalex +1 more source

