| 1. | Submillisecond radio pulsar
亚毫秒射电脉冲星
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| 2. | From this , most young radio pulsars are inferred to have magnetic fields between 1012 and 1013 gauss
从这个论点来推断，大部份年轻的无线电波霎应具有介于1012 ~ 1013高斯的磁场。
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| 3. | One ramification of our calculations is that radio pulsars are neutron stars in which the large - scale dynamo has failed to operate
从我们的计算中，还可以附带得到一点：无线电波霎正是无法形成大尺度发电机的中子星。
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| 4. | Yet the march 1979 burster , with an apparent rotation period of eight seconds , was spinning much more slowly than any radio pulsar then known
但1979年3月那次的爆炸源，看起来却有八秒的周期，自转速率要比当时所知的任何波霎还要慢得多。
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| 5. | The spin - down rate has been measured for almost every radio pulsar , and theory indicates that it depends on the strength of the star ' s magnetic field
这种自转变慢的速率，几乎每一颗无线电波霎都量得到，而理论指出，此速率和星体的磁场强度有关。
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| 6. | If the moving fluid in a newborn neutron star also transfers a tenth of its kinetic energy to the magnetic field , then the field would grow stronger than 1015 gauss , which is more than 1 , 000 times as strong as the fields of most radio pulsars
如果在新生中子星里的流体，也把10 %的动能转变成磁场的话，磁场强度会上涨到超过1015高斯，这是大多数无线电波霎所带磁场强度的1000倍以上。
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