The full evolution of the type-C quasi-periodic oscillations in MAXI J1348–630 revealed by Insight-HXMT

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
X.-L. Wang, Z. Yan, F.-G. Xie, J.-F. Wang, Y.-X. Li, Z.-Y. Liu, R.-Y. Ma
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Abstract

Context. Type-C quasi-periodic oscillations (QPOs) in black hole X-ray binaries serve as sensitive probes of accretion geometry and variability, although their full evolution throughout the entire outburst and the physics driving the evolution are not yet fully understood.Aims. Utilizing the intensive, broadband observations by Insight-HXMT of MAXI J1348−630, we aim to comprehensively investigate the properties and evolution of type-C QPOs during both its main 2019 outburst and subsequent mini-outbursts.Methods. We performed a comprehensive timing and spectral analysis of Insight-HXMT data. The evolution of QPO frequency, fractional rms, and energy dependence was tracked across spectral states, and correlations with X-ray flux and spectral shape were examined.Results. (1) The type-C QPO frequency rose from 0.24 Hz to 7.28 Hz during the main outburst rise and subsequently exhibited a nearly constant value of ∼7 Hz when the QPOs reappeared across different spectral states. (2) The fractional rms spectrum underwent a pronounced hardening following the transition from the hard to the hard-intermediate state. (3) The correlation between QPO frequency and X-ray flux exhibited strong hysteresis between the rise and decay phases; notably, the hysteresis loop reversed direction between the main and mini-outbursts. (4) In contrast, the frequency and hardness followed a tight, nearly single-track anticorrelation.Conclusions. Our results provide a complete picture of type-C QPO evolution. The stable reappearance frequency at ∼7 Hz indicates that the Compton region may reform at a consistent characteristic scale across different spectral states. Results (3) and (4) suggest that the type-C QPO frequency evolution is governed more by spectral shape than by X-ray luminosity, while the reversed hysteresis provides a new perspective on the differences between the main and mini-outbursts, possibly originating from variations in the initial conditions.
Insight-HXMT揭示的MAXI J1348-630中c型准周期振荡的完整演化
上下文。黑洞x射线双星中的c型准周期振荡(QPOs)是吸积几何和变异性的敏感探针,尽管它们在整个爆发过程中的完整演化以及驱动演化的物理机制尚未完全了解。利用MAXI J1348−630的Insight-HXMT的密集、宽带观测,我们旨在全面研究type-C QPOs在2019年主爆发和随后的小型爆发期间的性质和演化。我们对Insight-HXMT数据进行了全面的时序和光谱分析。QPO频率、分数均方根和能量依赖的演变在不同的光谱状态下被跟踪,并与x射线通量和光谱形状的相关性进行了研究。(1) c型QPO频率在主突上升期间从0.24 Hz上升到7.28 Hz,随后当QPO在不同谱态中再次出现时,其频率几乎保持在恒定的~ 7 Hz。(2)分数均方根谱在从硬态到硬中间态转变后发生了明显的硬化。(3) QPO频率与x射线通量的相关性在上升相和衰减相之间表现出较强的滞后性;值得注意的是,在主爆发和小爆发之间,磁滞回线的方向发生了反转。(4)频率与硬度呈紧密的单轨反相关关系。我们的结果提供了c型QPO进化的完整图景。在~ 7 Hz的稳定再现频率表明康普顿区域可以在不同的光谱状态下以一致的特征尺度进行重构。结果(3)和(4)表明,c型QPO频率的演变更多地受光谱形状而不是x射线亮度的控制,而反向迟滞则为研究主爆发和小爆发之间的差异提供了新的视角,这些差异可能源于初始条件的变化。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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