中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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; Yan Baorong; Zhao Chengshi; Yin Dongshang; Zhao Shuhong; Yang Tinggao; Gao Yuping
刊名Chinese Physics Letters
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

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。