关于积累流的起源,光子指数与近周期振荡频率 (Γ-vQPO) 的关系
Ambrose C Eze1, Romanus N C Eze2, Augustine E Chukwude2
1Department of Physics and Geosciences, Faculty of Natural Sciences and Environmental Studies, Godfrey Okoye University, Enugu, Nigeria. ceze@gouni.edu.ng.
Scientific reports
|April 4, 2025
概括
该研究分析了MAXI J1535-571的研究结果.
科学领域:
- 高能天体物理学 高能天体物理学
- X射线天文学X射线天文学
- 积累物理学的物理学
背景情况:
- MAXI J1535-571 呈现出具有相互连接的光谱时间特征的戏剧性爆发.
- 了解积聚流动力学对于黑洞和中子星研究至关重要.
研究的目的:
- 使用SWIFT/BAT和MAXI/GSC数据分析MAXI J1535-571的积累流特性.
- 为了研究光子指数和准周期性振荡 (QPO) 频率 (Γ-vQPO) 之间的关系.
主要方法:
- 分析了来自SWIFT/BAT和MAXI/GSC的数据.
- 使用XSPEC v12.10.1f.f.对数据进行了物理和现象模型的调整.
- 确定了积累流特征和 Γ-vQPO 关系.
主要成果:
- 共振条件表明可比的增积流时间尺度.
- 获得了近周期性振荡 (QPO) 频率,证实了双组分辅向流 (TCAF) 模型的预测.
- 发现积流速是反相关的,表明不同距离的相互作用.
- 在光子指数和QPO频率之间发现了密切的相关性 (系数为0.973).
结论:
- 这项研究证实了TCAF模型在硬光谱状态下对QPO的预测.
- 积累流速的变化似乎是驱动在硬介质光谱状态下 Γ-vQPO 关系的主要机制.
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