循环射电脉冲星

A. Lyne
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引用次数: 0

摘要

我们回顾了主要为发现循环脉冲星而设计的各种无线电调查。自第一颗毫秒脉冲星PSR 1937+21被发现以来的11年里,总共发现了大约55颗毫秒脉冲星,尽管其中大多数是在1988年以后才被发现的。大约在那个时候,第一颗毫秒脉冲星在一个球状星团中被发现,到目前为止,在这些天体中总共发现了34颗脉冲星。其中包括29颗周期小于50毫秒的脉冲星,14颗属于双星系统。新的星系调查已经发现了21颗毫秒脉冲星,其中大部分是在过去两年中发现的。它们构成了一个非常接近的星族,其空间密度与普通脉冲星相似。然而,它们的形成速度仅为每104-105年一次。
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Recycled radio pulsars
We review the various radio surveys which have been designed primarily for discovering recycled pulsars. In the 11 years since the first millisecond pulsar, PSR 1937+21, was found, a total of about 55 have been discovered, although most of these have only been found since 1988. Around that time, the first millisecond pulsar was found in a globular cluster and by now a total of 34 pulsars have been found in these objects. These include a total of 29 pulsars with period less than 50 ms and 14 are in binary systems. New galactic surveys have now discovered 21 millisecond pulsars, mostly discovered in the past 2 years. These constitute a very nearby population which has a space density similar to that of normal pulsars. However, their formation rate is only one every 104–105 years.
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