Kouveliotou C
Universities Space Research Association, ES-84, National Air and Space Administration/Marshall Space Flight Center, Huntsville, AL 35812, USA.
Proc Natl Acad Sci U S A. 1999 May 11;96(10):5351-2. doi: 10.1073/pnas.96.10.5351.
Recent x-ray observations have shown that a substantial fraction of newly born neutron stars have magnetic fields of several 10(14) G. They reveal themselves as soft gamma repeaters and anomalous x-ray pulsars and may account for the missing radio pulsars in young supernova remnants.
最近的X射线观测表明,相当一部分新诞生的中子星具有高达10的14次方高斯的磁场。它们以软伽马射线重复源和反常X射线脉冲星的形式出现,可能解释了年轻超新星遗迹中失踪的射电脉冲星的问题。