We provided a comprehensive study of the properties of the black hole in the low-mass X-ray binary system 4U 1543-47, specifically focusing on the 2021 outburst (MJD 59380-59470). Using observations from the \textit{Insight}-HXMT mission, we employed X-ray reflection fitting method and analyzed spectral data to estimate key black hole parameters. Through our investigation redbased on 6 out of the 52 available observations, we estimated the spin parameter of the black hole to be 0.902−0.053+0.054 and the inclination angle of the accretion disk to be 28.91−1.24+1.82 degrees (90\% confidence limits, statistical only), then we discussed the influence of high luminosity. Based on the \texttt{relxill} series models are not suitable for thick disk scenario, and in comparison with findings from other studies, we propose that our estimation of the spin value may be exaggerated.
@article{arxiv.2406.16292,
title = {Measuring the Spin of Black Hole Transient 4U 1543-47 Using Insight-HXMT},
author = {Jun Yang and Nan Jia and Erlin Qiao and Yujia Song and Lijun Gou},
journal= {arXiv preprint arXiv:2406.16292},
year = {2024}
}
Comments
11 pages, 10 figures, 5 tables, Accepted for publication in MNRAS