Infrared, submillimeter, and millimeter observations of the soft gamma repeaters

Details Infrared, submillimeter, and millimeter observations of the soft gamma repeaters Infrared, submillimeter, and millimeter observations of the soft gamma repeaters

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..966s&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 966-972 (1996).

Astronomy and Astrophysics

Astronomy

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

Scientific paper

The spectra of the quiescent counterparts to the Soft Gamma Repeaters SGR 1900+14 and SGR 1806-20 peak in the infrared, while they have not been detected at submillimeter or millimeter wavelengths. Their infrared spectra appear to contain several components: the photospheric emission from star(s) dominates at shorter wavelengths, a bright point source dominates at 25 μm, while an extended source dominates at 60 μm. The far infrared emission detected from SGR 0525-66 is consistent with that expected from heated dust in the supernova remnant N49. We review our latest millimeter, submillimeter, and infrared observations, and outline our plans for the future.

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