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GX 339-4中C型准周期振荡肩成分的交叉光谱分析

Cross-spectral Analysis of the Type-C Quasi-periodic Oscillation Shoulder Component in GX 339-4

Haifan Zhu, Mariano Méndez, Pengcheng Yang, Pei Jin, Candela Bellavita, Federico García, Wei Wang, Diego Altamirano, Liang Zhang, Chenxu Gao, Xiao Chen

arXiv 2608.12966首次发表:更新:

AI 中文总结

通过分析RXTE对GX 339-4的观测数据,采用联合PDS-CS分解方法,发现C型QPO的肩成分,其特性与B型QPO相似,或与B型QPO的早期宽变异性阶段相关。

AI 中文摘要

我们重新分析了Rossi X射线计时探测器(RXTE)在GX 339-4 2006/2007年爆发上升阶段的观测数据,并将联合功率密度谱(PDS)-交叉谱(CS)分解应用于C型准周期振荡(QPO)区域。在该框架下,QPO区域由一个窄的QPO基频和相邻的高频肩成分描述,可分别测量它们的振幅和相位滞后。该肩成分首次在MJD 54142.04被探测到,主要通过交叉谱的虚部和相位滞后谱中的窄局域结构,之后在功率密度谱中成为可分辨的高频肩成分。它在高频侧遵循QPO的频率演化,频率比R_ν=ν_sh/ν_QPO≈1.04-1.18。QPO的滞后保持较小,通常低于~0.17 rad,而肩成分携带更大的硬滞后,约0.5-0.8 rad。能量分辨拟合显示出相同的分离:在大部分能量带中,QPO滞后接近零或仅弱为正,而肩成分滞后系统性更大,且通常随光子能量增加。两个成分的均方根-能量形态大致相似,尽管它们的相对强度在观测序列中演化。尽管肩成分仍较宽,品质因数Q≈2-4,但其滞后和均方根-能量行为类似于我们观测后不久探测到的B型QPO。这种相似性提出了一种有趣的可能性,即该肩成分与后来被视为B型QPO的变异性的更早、更宽阶段相关。

英文摘要

We revisit Rossi X-ray Timing Explorer (RXTE) observations of GX~339$-$4 during the rising phase of its 2006/2007 outburst and apply a joint power-density-spectrum (PDS)--cross-spectrum (CS) decomposition to the type-C quasi-periodic oscillation (QPO) region. Within this framework, the QPO region is described by a narrow QPO fundamental and a neighboring high-frequency shoulder, whose amplitudes and phase lags can be measured separately. The shoulder is first detected at MJD~54142.04, mainly through the imaginary part of the CS and a narrow local structure in the phase-lag spectrum, before becoming a resolved high-frequency shoulder in the PDS. It follows the QPO frequency evolution on the high-frequency side, with $R_ν=ν_{\rm sh}/ν_{\rm QPO}\simeq1.04$--$1.18$. The QPO lag remains small, typically below $\sim0.17$~rad, whereas the shoulder carries a larger hard lag of $\sim0.5$--$0.8$~rad. Energy-resolved fits show the same separation: the QPO lag is close to zero or only weakly positive across most of the energy band, while the shoulder lag is systematically larger and generally increases with photon energy. The two components have broadly similar rms--energy shapes, although their relative strengths evolve during the observed sequence. Although the shoulder remains broad, with $Q\sim2$--$4$, its lag and rms--energy behavior resemble those of the type-B QPO detected shortly after our observations. This similarity raises the interesting possibility that the shoulder is related to an earlier, broader stage of the variability later seen as the type-B QPO.

Comments17 pages, 19 figures (including appendices). Accepted for A\&A

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