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Magnetar-like X-ray Bursts from a Rotation Powered Pulsar, PSR J1119-6127

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arxiv 1608.07133 v3 pith:ZMZ4YW4L submitted 2016-08-25 astro-ph.HE

Ersin Gogus , Lin Lin , Yuki Kaneko , Chryssa Kouveliotou , Anna L. Watts , Manoneeta Chakraborty , M. Ali Alpar , Daniela Huppenkothen
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Oliver J. Roberts George Younes Alexander J. van der Horst
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keywords burstsj1119-6127pulsarx-raybursteventsherepowered
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Two energetic hard X-ray bursts have recently triggered the Fermi and Swift space observatories from the rotation powered pulsar, PSR J1119-6127. We have performed in depth spectral and temporal analyses of these two events. Our extensive searches in both observatory data for lower luminosity bursts uncovered 10 additional events from the source. We report here on the timing and energetics of the 12 bursts from PSR J1119-6127 during its burst active phase of 2016 July 26 and 28. We also found a spectral softer X-ray flux enhancement in a post burst episode, which shows evidence of cooling. We discuss here the implications of these results on the nature of this unusual high-field radio pulsar, which firmly place it within the typical magnetar population.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 62 citations worldwide. Full citation record

  1. Searching for links between energetic millisecond pulsars and repeating fast radio bursts

    astro-ph.HE 2026-05 unverdicted novelty 4.0 of 10

    Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.

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