volume 13, issue S337, P104-107 2017
DOI: 10.1017/s1743921317010304
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A. Borghese, N. Rea, F. Coti Zelati, P. Esposito

Abstract: Abstract1E 161348-5055 (1E 1613), the source at the center of the supernova remnant RCW 103, has defied any easy classification since its discovery, owing to its long-term variability (a factor of ~ 100 in flux on time scales from months to years) and a periodicity of 6.67 hr with a variable light curve profile across different flux levels. On June 2016, 1E 1613 emitted a magnetar-like millisecond burst of hard X-rays accompanied with a factor ~ 100 brightening in the persistent soft X-ray emission. The durati…

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