The fine spectral structure of Cygnus X-1
文献类型:期刊论文
作者 | Li C(李晨); Li TB(李惕碚)![]() ![]() |
刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
![]() |
出版日期 | 2000 |
卷号 | 24期号:3页码:#REF! |
关键词 | Cyg X-1 X-ray LSSM power spectral density |
通讯作者 | Chen, L (reprint author), Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China. |
英文摘要 | The power spectral density (PSD) of Cyg X-l is divided into two parts by using the linear state space model (LSSM). One part is the PSD of LSSM, the other is the residual power spectral density (RPSD) defined by the whole PSD minus the model PSD. We focus our attention on analyzing the RPSD. The results show that RPSD has different characteristics in 3 different states-the low/hard, transition and high/soft states. There is a broad peak structure both in the high/soft and low/hard states, with average central frequencies similar to 8Hz and similar to 5 HZ respectively The RPSD in the low/hard state may peak at similar to 0.07 HE. While during the Transition State, the RPSD has a double-peak structure, with the central frequencies in the regions of 0.5-4Hz and 5-11Hz respectively and these are quite close to the QPO central frequencies we have previously obtained. This fact implies that the QPO and the auto-regression that is needed in LSSM belong to different physical processes. Comparing to PSD, the RPSD is more sensitive to variations, such as the QPO, the broken frequencies and so on, The reason for the variable peak in the RPSD is discussed. |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
收录类别 | SCI |
WOS记录号 | WOS:000088821200006 |
公开日期 | 2016-05-03 |
源URL | [http://ir.ihep.ac.cn/handle/311005/227489] ![]() |
专题 | 高能物理研究所_院士 |
推荐引用方式 GB/T 7714 | Li C,Li TB,Song LM,et al. The fine spectral structure of Cygnus X-1[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2000,24(3):#REF!. |
APA | 李晨.,李惕碚.,宋黎明.,冯育新.,Chen, L.,...&Feng, YX.(2000).The fine spectral structure of Cygnus X-1.CHINESE ASTRONOMY AND ASTROPHYSICS,24(3),#REF!. |
MLA | 李晨,et al."The fine spectral structure of Cygnus X-1".CHINESE ASTRONOMY AND ASTROPHYSICS 24.3(2000):#REF!. |
入库方式: OAI收割
来源:高能物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。