# A MAGNETAR-LIKE OUTBURST FROM A HIGH-B RADIO PULSAR

@article{Archibald2016AMO,
title={A MAGNETAR-LIKE OUTBURST FROM A HIGH-B RADIO PULSAR},
author={Robert F. Archibald and Victoria M. Kaspi and Shriharsh P. Tendulkar and Paul Scholz},
journal={The Astrophysical Journal Letters},
year={2016},
volume={829}
}
• Published 2 August 2016
• Physics
• The Astrophysical Journal Letters
Radio pulsars are believed to have their emission powered by the loss of rotational kinetic energy. By contrast, magnetars show intense X-ray and γ-ray radiation whose luminosity greatly exceeds that due to spin down and magnetar luminosity is believed to be powered by intense internal magnetic fields. A basic prediction of this picture is that radio pulsars of high magnetic field should show magnetar-like emission. Here we report on a magnetar-like X-ray outburst from the radio pulsar PSR…
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