Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits
文献类型:期刊论文
作者 | Tong Minglei![]() ![]() ![]() ![]() ![]() ![]() |
刊名 | Chinese Physics Letters
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出版日期 | 2013 |
卷号 | 30期号:11页码:119901 |
ISSN号 | 0256-307X |
英文摘要 | One regrettable error appeared in Eq. (21) of our article Chin. Phys. Lett. 30 (2013) 100402. The correct one of the equation is as follows: One can estimate the frequency difference now replaced to be δ? ≈ 10~(?11) Hz, which is two orders of magnitude lower than the frequency resolution of PTAs. Hence, we can ignore the evolution effects of the binary in OJ287 in this study. |
语种 | 英语 |
源URL | [http://210.72.145.45/handle/361003/9021] ![]() |
专题 | 国家授时中心_守时理论与方法研究室 |
作者单位 | 中国科学院国家授时中心 |
推荐引用方式 GB/T 7714 | Tong Minglei,Yan Baorong,Zhao Chengshi,et al. Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits[J]. Chinese Physics Letters,2013,30(11):119901. |
APA | Tong Minglei.,Yan Baorong.,Zhao Chengshi.,Yin Dongshang.,Zhao Shuhong.,...&Gao Yuping.(2013).Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits.Chinese Physics Letters,30(11),119901. |
MLA | Tong Minglei,et al."Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits".Chinese Physics Letters 30.11(2013):119901. |
入库方式: OAI收割
来源:国家授时中心
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