An analysis of the X-ray emission in the late stage of SN 1987 A |
| |
| Institution: | Department of Applied Physics, Shanghai Jiaotong University, Shanghai 200240 ROC;Department of Biomedical Engineering, The Hong Kong Polytechnic University, Kowloon, Hong Kong SAR, P.R. China |
| |
| Abstract: | 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. |
| |
| Keywords: | |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
