Aug 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....4...40c&link_type=abstract
Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o
Physics
Scientific paper
We have derived a new, precise position for the Soft Gamma Repeater SGR1806-20 by triangulating eight bursts observed by Ulysses, BATSE, and KONUS-WIND. The resulting error box, although within the radio contours of the Galactic supernova remnant G10.0-0.3, is significantly displaced from its core. Although this can be explained by a high velocity neutron star, it raises interesting questions about the model of SGR emission from this object.
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