Abstract
AN important clue to the nature of soft γ-ray repeaters (SGRs), which emit recurrent bursts of γ-rays, has been provided by the association of two of the three known SGRs with supernova remnants1,2 (SNRs). Here we present radio images of the non-thermal radio nebula G10.0 – 0.3, a supernova remnant which has been associated previously2 with SGR1806 – 20 (refs 3, 4). Our images show that the nebula is a plerion (that is, the radio emission is synchrotron radiation powered by a central pulsar), as revealed by the observation of a hierarchy of nested shells and a bright central peak. The recent detection5 of an X-ray point source coincident with the radio peak and of a hard X-ray burst5,6 from G10.0 – 0.3 confirms the SGR–SNR association. We propose that SGR1806 – 20 is an isolated pulsar that emits both steady and impulsive winds of relativistic particles, which together power the nebula. We suggest that the offset from the centres of the SNRs observed for both this object and SGR0526 – 66 (ref. 1), requiring high velocities of the pulsars, provides a clue to their formation mechanism.
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Kulkarni, S., Frail, D., Kassim, N. et al. The radio nebula of the soft γ-ray repeater 1806 – 20. Nature 368, 129–131 (1994). https://doi.org/10.1038/368129a0
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DOI: https://doi.org/10.1038/368129a0
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