X-ray spectral and timing evolution during the 2018 outburst of MAXI J1820+070
YaXing Li, Zhen Yan, ChenXu Gao, Wenfei Yu

TL;DR
This study analyzes the spectral and timing evolution of MAXI J1820+070 during its 2018 outburst using high-cadence X-ray observations, revealing unique spectral state transitions, correlations between QPOs and spectral parameters, and jet ejection timing.
Contribution
It provides detailed insights into the spectral-timing evolution and the coupling between QPO properties and Comptonization processes in a black hole X-ray binary during outburst.
Findings
The HID shows a 'q'-like track with a unique loop in the hard state.
A negative correlation between QPO frequency and optical depth was observed.
The last QPO detection coincides with a transient jet ejection within one hour.
Abstract
We made use high-cadence observations from the -HXMT and to scrutinize the spectral and timing evolution during the 2018 outburst of the black hole X-ray binary (BHXRB) MAXI J1820+070. It's hardness-intensity diagram (HID) displays a ``q''-like track including all the spectral states, along a unique loop in the hard state. The tracks observed in the HID is anticipated in the evolution of the components responsible for Compton and reflection emission. This is substantiated by the relationship between the X-ray luminosity and photon index which exhibits a pattern reminiscent of HID. The distinctive evolution of the reflection component leads to the unique loop in the HID (also in the -- plane) of hard state. Additionally, we found a negative correlation between frequency of the type-C quasi-periodic oscillation (QPO)…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Gamma-ray bursts and supernovae
