标题： 射电脉冲星是AXP和SGR的前身吗？ 显示英文标题

标题： Are radio pulsars progenitors of AXPs and SGRs?

摘要： 分析了起源于射电脉冲星的磁层活动周期天体（AXPs）和软伽马重复源（SGRs）的场景实现的可能性，这些射电脉冲星经历了频繁且强烈的脉冲幅度突然变化。 结果表明，作为AXPs和SGRs可能前身的这类脉冲星，与超新星遗迹（SNRs）的关联及其在$P - \dot P$图表上的演化，考虑其实际年龄后，与提出的场景存在冲突。 显示英文摘要

摘要： Possibility of realization of scenario for the AXPs and SGRs origins from radio pulsars, which were undergone frequent and strong glitches, was analyzed. It is shown that the characteristics of such pulsars - the possible progenitors of AXPs and SGRs - their association with supernova remnants (SNRs) and evolution on the $P - \dot P$ diagram, taking into account their real ages, conflict with offered scenario.