Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits

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	Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits
	Tong Minglei; Yan Baorong; Zhao Chengshi; Yin Dongshang; Zhao Shuhong; Yang Tinggao; Gao Yuping
	2013
发表期刊	Chinese Physics Letters
ISSN	0256-307X
卷号	30 期号:11 页码:119901
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.
收录类别	SCI
语种	英语
文献类型	期刊论文
条目标识符	http://210.72.145.45/handle/361003/9021
专题	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
第一作者单位	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.

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