Hessels Jason W T, Ransom Scott M, Stairs Ingrid H, Freire Paulo C C, Kaspi Victoria M, Camilo Fernando
Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada.
Science. 2006 Mar 31;311(5769):1901-4. doi: 10.1126/science.1123430. Epub 2006 Jan 12.
We have discovered a 716-hertz eclipsing binary radio pulsar in the globular cluster Terzan 5 using the Green Bank Telescope. It is the fastest spinning neutron star found to date, breaking the 24-year record held by the 642-hertz pulsar B1937+21. The difficulty in detecting this pulsar, because of its very low flux density and high eclipse fraction (approximately 40% of the orbit), suggests that even faster spinning neutron stars exist. If the pulsar has a mass less than twice the mass of the Sun, then its radius must be constrained by the spin rate to be <16 kilometers. The short period of this pulsar also constrains models that suggest that gravitational radiation, through an r-mode (Rossby wave) instability, limits the maximum spin frequency of neutron stars.
我们使用绿岸望远镜在球状星团特赞5中发现了一颗频率为716赫兹的食双星射电脉冲星。它是迄今为止发现的自转最快的中子星,打破了频率为642赫兹的脉冲星B1937+21保持了24年的记录。由于该脉冲星的流量密度非常低且食分很高(约占轨道的40%),探测它存在困难,这表明可能存在自转更快的中子星。如果该脉冲星的质量小于太阳质量的两倍,那么其半径必然受自转速率限制而小于16千米。这颗脉冲星的短周期也对一些模型提出了限制,这些模型认为引力辐射通过r模(罗斯比波)不稳定性限制了中子星的最大自旋频率。