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Measuring the Spin of Black Hole Transient 4U 1543-47 Using Insight-HXMT

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arxiv 2406.16292 v1 pith:SAHF27WL submitted 2024-06-24 astro-ph.HE

classification astro-ph.HE
keywords blackholespindiskobservationsx-rayaccretionanalyzed
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abstract

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.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Radio flares and X-ray hardening embedded in the long soft state of 4U 1543-475

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    Radio flares in 4U 1543-475 coincided with X-ray hardening, enhanced coronal emission, and lower reflection fraction, suggesting transient inner-disk changes accompany jet launching.

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