摘要
估算了球状星团４７Ｔｕｃａｎａｃ中由脉冲星自转所辐射的高频引力波和由双星绕转所辐射的低频引力波的总功率、地面流量以及谱分布．最后，讨论了探测的可行性．
In this paper, the gravitational wave luminosity, energy flux and the spectral density of the strain amplitude of both the high frequency due to the rotation of the millisecond plsar and the low frequency hue to the orbital rotation of binary pulsars are estimated respectively. Finally the probability of detection is discussed.
关键词
引力辐射
球状星团
毫秒级
脉冲星
Gravitational Radiation, Globular cluster, Millisecond pulsar.
