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

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ID: 324371
2026
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Abstract
Abstract We present a comprehensive multi-wavelength study of the black hole X-ray binary 4U 1543–475 during its 2021 outburst, focusing on radio flaring episodes that are commonly interpreted as signatures of episodic jet production and are embedded within states when the X-ray emission was dominated by an accretion disk component. The radio monitoring reveals at least two discrete flares that coincide with periods of enhanced Comptonized X-ray emission. Broadband spectral modelling shows a significant decrease in the reflection-to-disk flux ratio (by a factor of ~3 − 4) during these episodes, consistent with a temporary change in the geometry of the inner accretion flow, although the data do not allow the causal sequence to be firmly established. Optical photometry exhibits variability that broadly tracks the reflection fraction, consistent with changes in the illuminating component. The accompanying spectral hardening indicates that the radio flares were associated with short-lived excursions toward a ”harder” state, departing from the soft state. X-ray timing analysis suggests that the radio flares may be associated with changes in the fractional rms variability; however, no consistent or unified pattern can be firmly established across different events. These results provide a multi-wavelength observational example of radio flaring activity in a black hole binary and highlight the complex interplay between accretion flow geometry, coronal emission, and jet-related phenomena.
Reference Key
openalex_W7201980347 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors Zuobin Zhang, Rob Fender, Jiachen Jiang, Payaswini Saikia, D. M. Russell, Andrew Hughes, Honghui Liu, Francesco Carotenuto, James F Steiner, F. J. Cowie, John A Tomsick, Cosimo Bambi, Yimin Huang, Xian Zhang, Wenfei Yu, Yuexin Zhang, Rittick Roy
Journal monthly notices of the royal astronomical society
Year 2026
DOI
10.1093/mnras/stag1470
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