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radio pulsar 【天文學】射電腦衛星。

radio quiet

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體,也把10 %的動能轉變成磁場的話,磁場強度會上漲到超過1015高斯,這是大多數無線電波霎所帶磁場強度的1000倍以上。

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 這種自轉變慢的速率,幾乎每一顆無線電波霎都量得到,而理論指出,此速率和星體的磁場強度有關。

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,看起來卻有八秒的周期,自轉速率要比當時所知的任何波霎還要慢得多。

One ramification of our calculations is that radio pulsars are neutron stars in which the large - scale dynamo has failed to operate 從我們的計算中,還可以附帶得到一點:無線電波霎正是無法形成大尺度發電機的中子星。

From this , most young radio pulsars are inferred to have magnetic fields between 1012 and 1013 gauss 從這個論點來推斷,大部份年輕的無線電波霎應具有介于1012 ~ 1013高斯的磁場。

Submillisecond radio pulsar 亞毫秒射電脈沖星