Hard X-rays from supernova 1987A - Results of observations performed with the Roentgen observatory onboard the KVANT module during 1987-1989

Astronomy and Astrophysics – Astronomy

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Abundance, Brightness Distribution, Supernova 1987A, X Ray Spectra, Annual Variations, Cobalt Isotopes, Light Curve, X Ray Astronomy

Scientific paper

Observations performed with the Hexe instrument onboard the Kvant module indicate that, by May-June 1989, the hard X-ray flux from SN1987 had declined by more than a factor of 8 compared with the maximum of the X-ray light curve. The upper limits to the Co-57/Co-56 abundance ratio at the level of three standard deviations was obtained. The value of this ratio exceeds that of the Fe-57/Fe-56 ratio on earth by a factor of 1.5.

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