Results 171 to 180 of about 54,876 (252)
Diagnosing the Particle Transport Mechanism in the Pulsar Halo via X-Ray Observations
Pulsar halos (also termed “TeV halos”) are a new class of γ -ray sources in the Galaxy, which manifest as extended γ -ray emission around middle-aged pulsars, as discovered around the Geminga pulsar, the Monogem pulsar, and PSR J0622+3749 by the High ...
Qi-Zuo Wu+4 more
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Energy dependent γ-ray morphology in the pulsar wind nebula HESS J1825–137 [PDF]
F. Aharonian+99 more
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Special Issue "Synthetic Aperture Radar (SAR) Techniques and Applications". [PDF]
Bovenga F.
europepmc +1 more source
We obtained a 108 ks Chandra X-ray Observatory (CXO) observation of PSR J1849-0001 and its pulsar wind nebula (PWN) coincident with the TeV source HESS J1849-000.
Seth Gagnon+6 more
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From Supernova to Remnant: Tracking the Evolution of the Oldest Known X-Ray Supernovae. [PDF]
Ramakrishnan V, Dwarkadas VV.
europepmc +1 more source
X‐Ray Emission from PSR J1809−1917 and Its Pulsar Wind Nebula, Possibly Associated with the TeV Gamma‐Ray Source HESS J1809−193 [PDF]
Oleg Kargaltsev, George G. Pavlov
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This paper investigates the origin of the γ -ray emission from MGRO J1908+06 in the GeV–TeV energy band. By analyzing the data collected by the Fermi Large Area Telescope, the Very Energetic Radiation Imaging Telescope Array System, and High Altitude ...
A. Acharyya+129 more
doaj +1 more source
A new interesting source in Chandra field: a pulsar wind nebula? [PDF]
Sudip Bhattacharyya
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DISTANCE DETERMINATION TO THE CRAB-LIKE PULSAR WIND NEBULA G54.1+0.3 AND THE SEARCH FOR ITS SUPERNOVA REMNANT SHELL [PDF]
D. A. Leahy, W. W. Tian, Q. Daniel Wang
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Optical identification of the 3C 58 pulsar wind nebula [PDF]
Yu. A. Shibanov+4 more
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