The emission positions of kHz QPOs and Kerr spacetime influence
文献类型：期刊论文
| 作者 | Zhang ChengMin1 ; Wei YingChun1; Yin HongXing1; Zhao YongHeng1; Lei YaJuan2; Song LiMing2; Zhang Fan2; Yan Yan3
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| 刊名 | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
 |
| 出版日期 | 2010 |
| 卷号 | 53页码:114-116 |
| 关键词 | kHz QPO neutron star low-mass X-ray binaries |
| 英文摘要 | Based the Alfven wave oscillation model (AWOM) and relativistic precession model (RPM) for twin kHz QPOs, we estimate the emission positions of most detected kHz QPOs to be at r=18+/-3 km (R/15 km), except Cir X-1 at r similar to 30+/-5 km (R/15 km). For the proposed Keplerian frequency as an upper limit to kHz QPO, the spin effects in Kerr Spacetime are discussed, which have about a 5% (2%) modification for that of the Schwarzchild case for the spin frequency of 1000 (400) Hz. The application to the four typical QPO sources, Cir X-1, Sco X-1, SAX J1808.4-3658 and XTE 1807-294, is mentioned. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000280291800026 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/7723]  |
| 专题 | 国家天文台_应用天文研究部 |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China 3.CAS, Natl Astron Observ, Urumqi Observ, Urumqi 830011, Peoples R China |
| 推荐引用方式 GB/T 7714 | Zhang ChengMin,Wei YingChun,Yin HongXing,et al. The emission positions of kHz QPOs and Kerr spacetime influence[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2010,53:114-116. |
| APA | Zhang ChengMin.,Wei YingChun.,Yin HongXing.,Zhao YongHeng.,Lei YaJuan.,...&Yan Yan.(2010).The emission positions of kHz QPOs and Kerr spacetime influence.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,53,114-116. |
| MLA | Zhang ChengMin,et al."The emission positions of kHz QPOs and Kerr spacetime influence".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 53(2010):114-116. |
入库方式： OAI收割
来源：国家天文台
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