A possible IR/x-ray counterpart to SGR1900+14

Details A possible IR/x-ray counterpart to SGR1900+14 A possible IR/x-ray counterpart to SGR1900+14

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..366...74h&link_type=abstract

High velocity neutron stars and gamma-ray bursts. AIP Conference Proceedings, Volume 366, pp. 74-78 (1996).

Physics

2

Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray

Scientific paper

We present the results of deep ROSAT HRI observations of the region around the network synthesis position for the soft repeater SGR1900+14. The strongest x-ray source (0.1-2.4 keV flux 7×10-13 erg cm-2 s-1) has a position consistent with a small network synthesis error box and the KONUS localization for this source, as well as with a peculiar infrared source. The quiescent soft x-ray characteristics of the three SGR's appear to differ widely.

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