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Reactivation and Precise IPN Localization of the Soft Gamma Repeater SGR1900+14

K. Hurley·C. Kouveliotou·P. Woods·T. Cline·P. Butterworth·E. Mazets·S. Golenetskii·D. Frederics
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Abstract

In 1998 May, the soft gamma repeater SGR1900+14 emerged from several years of quiescence and emitted a series of intense bursts, one with a time history unlike any previously observed from this source. Triangulation using Ulysses, BATSE, and KONUS data give a 1.6 square arcminute error box near the galactic supernova remnant G42.8+0.6. This error box contains a quiescent soft X-ray source which is probably a neutron star associated with the soft repeater.

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K. Hurley, C. Kouveliotou, P. Woods, T. Cline, P. Butterworth, E. Mazets, S. Golenetskii, D. Frederics. 1998-11-25. Reactivation and Precise IPN Localization of the Soft Gamma Repeater SGR1900+14. https://doi.org/10.1086/311821

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