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

作者：Wu, H^*; Deng, JS; Shi, JR; You, JH

来源：Chinese Astronomy and Astrophysics, 1999, 23(1): 42-50.

DOI：10.1016/S0275-1062(99)00025-9

• SN 1987A
• thermal bremsstrahlung radiation

Following the reasonable explanation of the evolution of the SN 1987A'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.

• 出版日期1999-3
• 单位上海交通大学