Multiwavelength observations of the Soft Gamma-Ray Repeaters

Details Multiwavelength observations of the Soft Gamma-Ray Repeaters Multiwavelength observations of the Soft Gamma-Ray Repeaters

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..366...79s&link_type=abstract

High velocity neutron stars and gamma-ray bursts. AIP Conference Proceedings, Volume 366, pp. 79-83 (1996).

Astronomy and Astrophysics

Astronomy

1

Gamma-Ray Sources, Gamma-Ray Bursts, Astronomical Observations

Scientific paper

We present the current status of the multiwavelength observations of the quiescent counterparts to the Soft Gamma-Ray Repeaters, and out-line our future observing plans. The preliminary observations suggest that the plerion model is not appropriate for these sources. Instead, the combination of some form of dust emission with a non-thermal radio emission (in SGR1806-20) is more plausible.

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