Many of the recently discovered galactic very high-energy gamma-ray sources are
associated with Pulsar Wind Nebulae (PWN), which is the most populous source category
at TeV energies. Extended synchrotron nebulae seen from these objects in the X-ray
band is a footprint of the relativistic winds, generated by the young energetic
pulsars, which interact with the matter ejected by the supernova ex
...
More