Analysis of the soft X-ray emission of SN 1987A.

Details Analysis of the soft X-ray emission of SN 1987A. Analysis of the soft X-ray emission of SN 1987A.

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acaps..18..369w&link_type=abstract

Acta Astrophys. Sin., Vol. 18, No. 4, p. 369 - 376

Astronomy and Astrophysics

Astrophysics

Supernovae: X Rays, Supernovae: Bremsstrahlung

Scientific paper

Following the reasonable explanation of the evolution of the SN 1987A's bolometric luminosity at the later phase by the accretion model, the authors suggest that the observed soft X-ray originates in the accretion of the central neutron star. Results of their model calculation are consistent with the observations. They predict that the observed X-ray flux will increase only for a certain length of time, and will begin to decrease around day 4100.

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