Exploration of the origin of 2020 X-ray outburst in OJ 287
Shifeng Huang, Shaoming Hu, Hongxing Yin, Xu Chen, Sofya Alexeeva, and, Yunguo Jiang

TL;DR
This study investigates the 2020 X-ray outburst in OJ 287, comparing possible origins such as black hole-disc impact and tidal disruption events, and finds evidence supporting a TDE-related cause based on spectral and temporal analysis.
Contribution
The paper provides a comparative analysis of the 2020 outburst with previous events and introduces evidence favoring a tidal disruption event as the likely origin.
Findings
Spectral and hardness ratio correlations differ from quiescent state.
The 2020 outburst shares features with the 2016-2017 TDE candidate.
X-ray decay fits TDE models ($t^{-5/3}$ and $t^{-9/4}$).
Abstract
Research into OJ 287 has been ongoing for many years. In 2020 April-June, this source underwent the second highest X-ray outburst (second only to the 2016-2017 outburst) and the mechanism of this outburst is still under debate. In this paper, we discuss two scenarios to explore the origin of the outburst: an after-effect of a black hole-disc impact and a tidal disruption event (TDE). We present the weak correlations of the spectral index versus X-ray flux and the hardness ratio (HR) versus the soft X-ray flux during the outburst, and these features are different from the case in the quiescent state. The correlations are compared with those of the 2016-2017 outburst with the highest X-ray flux in monitoring history. Analysis of the outbursts in 2016-2017 and 2020 shows that the expected time of the X-ray outburst, based on the theory of the after-effect of the black hole-disc impact and…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Scientific Measurement and Uncertainty Evaluation · Mechanics and Biomechanics Studies
