Results 161 to 170 of about 8,336 (234)
Discovery of a New X‐Ray Filled Radio Supernova Remnant around the Pulsar Wind Nebula in 3EG J1809−2328 [PDF]
M. S. Roberts, C. L. Brogan
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Radio Observation of the Pulsar Wind Nebula in Supernova Remnant G11.2−0.3
Pulsar wind nebulae (PWNe) are important sources for understanding galactic high-energy processes, but it is controversial until now how high-energy particles in PWNe are accelerated and transported. Lacking radio counterparts of X-ray PWNe (the proposed
Yu Zhang+4 more
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A new interesting source in Chandra field: a pulsar wind nebula? [PDF]
Sudip Bhattacharyya
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First XMM-Newton results on the Pulsar Wind Nebula in the composite supernova remnant G0.9+0.1
D. Porquet+2 more
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The Crab pulsar and its pulsar-wind nebula in the optical and infrared [PDF]
A. Tziamtzis+2 more
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Testing a stochastic acceleration model of pulsar wind nebulae: early evolution of a wind nebula associated with SN 1986J [PDF]
Shuta Tanaka, Kazumi Kashiyama
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Multiband Nonthermal Radiative Study of PeVatron Candidate Pulsar Wind Nebula HESS J1849-000
Pulsar wind nebula HESS J1849-000 is one of the sources that may emit PeV γ -ray photons based on the recent measurement by the Tibet Air Shower Array and the Large High Altitude Air Shower Observatory.
Bo-Tao Zhu, Fang-Wu Lu, Li Zhang
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Subaru Telescope -History, active/adaptive optics, instruments, and scientific achievements. [PDF]
Iye M.
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