The high magnetic field pulsar PSR J1119-6127 shows a double-pulse profiles and RRAT-like emission after glitches. Otherwise, it looks like a normal pulsar. The RRAT-like emission appears as single pulses outside of the main pulse. Also the RRAT-like pulses move around in phase so these strong pulses don't show periodicity over the short integration span.
arXiv:1010.0857 [pdf, ps, other]
Title: The glitch-induced identity changes of PSR J1119-6127
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