X-ray emission from the young pulsar J1357-6429 and similar objects
Vyacheslav Zavlin (NASA/MSFC/USRA)
The first Chandra and XMM-Newton observations of the young and energetic pulsar J1357-6429 provided strong indications of a tail-like pulsar-wind nebula associated with this object, as well as pulsations of its X-ray flux with a pulsed fraction above 50