The photon-index-time-lag correlation in black hole X-ray binaries

被引:19
作者
Reig, Pablo [1 ,2 ,3 ]
Kylafis, Nikolaos D. [1 ,2 ,3 ]
Papadakis, Iossif E. [1 ,2 ,3 ]
Teresa Costado, Maria [4 ]
机构
[1] Fdn Res & Technol Hellas, IESL, Iraklion 71110, Greece
[2] Univ Crete, Phys Dept, Iraklion 70013, Greece
[3] Univ Crete, Inst Theoret & Computat Phys, Iraklion 70013, Greece
[4] CSIC, Inst Astrofis Andalucia, Apdo 3004, E-18080 Granada, Spain
关键词
stars: black holes; galaxies: jets; X-rays: binaries; LONG-TERM VARIABILITY; ADVECTION-DOMINATED ACCRETION; CYGNUS X-1; LOW/HARD STATE; HARD STATE; TIMING-EXPLORER; GX; 339-4; SPECTRAL EVOLUTION; TEMPORAL CORRELATIONS; RADIATION MECHANISM;
D O I
10.1093/mnras/stx2683
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have performed a timing and spectral analysis of a set of black hole binaries to study the correlation between the photon index and the time lag of the hard photons with respect to the soft ones. We provide further evidence that the timing and spectral properties in black hole X-ray binaries are coupled. In particular, we find that the average time lag increases as the X-ray emission becomes softer. Although a correlation between the hardness of the X-ray spectrum and the time (or phase) lag has been reported in the past for a handful of systems, our study confirms that this correlated behaviour is a global property of black hole X-ray binaries. We also demonstrate that the photon-index-time-lag correlation can be explained as a result of inverse Comptonization in a jet.
引用
收藏
页码:4644 / 4652
页数:9
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