Erratum:Pulsar Timing Residuals Induced by Gravitational Waves from Single Non-evolving Supermassive Black Hole Binaries with Elliptical Orbits[Chin.Phys.Lett.30(2013)100402]  

作　　者：TONG Ming-Lei YAN Bao-Rong ZHAO Cheng-Shi YIN Dong-Shang ZHAO Shu-Hong YANG Ting-Gao GAO Yu-Ping 童明雷;燕保荣;赵成仕;尹东山;赵书红;杨廷高;高玉平(National Time Service Center,Chinese Academy of Sciences,Xi'an 710600;Key Laboratory of Time and Frequency Primary Standards,Chinese Academy of Sciences,Xi'an 710600;Key Laboratory of Precision Navigation and Timing Technology,Chinese Academy of Sciences,Xi'an 710600)

机构地区：[1]National Time Service Center,Chinese Academy of Sciences,Xi'an 710600 [2]Key Laboratory of Time and Frequency Primary Standards,Chinese Academy of Sciences,Xi'an 710600 [3]Key Laboratory of Precision Navigation and Timing Technology,Chinese Academy of Sciences,Xi'an 710600

出　　处：《Chinese Physics Letters》2013年第11期220-220,共1页中国物理快报（英文版）

摘　　要：PACS:99.10.−x,04.30.Db,97.60.Gb,95.85.Sz DOI:10.1088/0256-307X/30/11/119901 One regrettable error appeared in Eq.(21)of our article[Chin.Phys.Lett.30(2013)100402].The cor-rect one of the equation is as follows.

关 键 词：massive Pulsar s 

分 类 号：P14[天文地球—天体物理]