An analysis of the X-ray emission in the late stage of SN 1987 A

Details An analysis of the X-ray emission in the late stage of SN 1987 A An analysis of the X-ray emission in the late stage of SN 1987 A

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cha%26a..23...42w&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 23, Issue 1, p. 42-50.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Following the reasonable explanation of the evolution of the SN 1987 A's bolometric luminosity at the later phase by the accretion model, we suggest that the observed soft X-ray originates in the accretion of the central neutron star. Results of our model calculation are consistent with the observations. We 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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