Hard X-ray Emission along the Z Track in GX 17+2
文献类型:期刊论文
作者 | Ding, G. Q.![]() ![]() |
刊名 | JOURNAL OF ASTROPHYSICS AND ASTRONOMY
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出版日期 | 2015-09-01 |
卷号 | 36期号:3页码:335-353 |
关键词 | Accretion: accretion disks X-rays: binaries stars: individual (GX 17+2) stars: neutron |
英文摘要 | Using the data from the Proportional Counter Array (PCA) and the High-Energy X-ray Timing Experiment (HEXTE) on board Rossi X-Ray Timing Explorer for Z source GX 17 + 2, we investigate the evolution of its PCA spectra and HEXTE spectra along a 'Z' track on its hardness-intensity diagram. A hard X-ray tail is detected in the HEXTE spectra. The detected hard X-ray tails are discontinuously scattered throughout the Z track. The found hard X-ray tail hardens from the horizontal branch, through the normal branch, to the flaring branch in principle and it contributes (20-50)% of the total flux in 20-200 keV. Our joint fitting results of the PCA + HEXTE spectra in 3-200 keV show that the portion of Comptonization in the Bulk-Motion Comptonization (BMC) model accounts for the hard X-ray tail, which indicates that the BMC process could be responsible for the detected hard tail. The temperature of the seed photons for BMC is 2.7 keV, implying that these seed photons might be emitted from the surface of the neutron star (NS) or the boundary layer between the NS and the disk and, therefore, this process could take place around the NS or in the boundary layer. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | ACCRETING BLACK-HOLES ; BROAD-BAND SPECTRUM ; COLOR-COLOR DIAGRAM ; CIRCINUS X-1 ; SCORPIUS X-1 ; CYGNUS X-2 ; OBSERVATIONAL EVIDENCE ; BEPPOSAX OBSERVATIONS ; RXTE OBSERVATIONS ; ENERGY-SPECTRA |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000361891800001 |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/889] ![]() |
专题 | 高能天体物理研究团组 |
作者单位 | Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China |
推荐引用方式 GB/T 7714 | Ding, G. Q.,Huang, C. P.. Hard X-ray Emission along the Z Track in GX 17+2[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2015,36(3):335-353. |
APA | Ding, G. Q.,&Huang, C. P..(2015).Hard X-ray Emission along the Z Track in GX 17+2.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,36(3),335-353. |
MLA | Ding, G. Q.,et al."Hard X-ray Emission along the Z Track in GX 17+2".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 36.3(2015):335-353. |
入库方式: OAI收割
来源:新疆天文台
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