论文标题
无线电脉冲星子选集（ii）：神秘的rrats
Radio Pulsar Sub-Populations (II) : The Mysterious RRATs
论文作者
论文摘要
已经提出了一些猜想，以解释rrats，中子恒星的最新子类及其与其他无线电脉冲星的联系。这项工作在RRAT人群的特征性能中讨论了这些猜想。与期望相反，可以看出 - a）RRAT种群在统计上与无效的脉冲星无关，b）rrat现象不太可能与老年或死亡线接近性有关。 rrats的特殊排放特性可能更有可能是它们后来成为其他类型的中子星的进化阶段的标志，这可能导致磁场的重组。
Several conjectures have been put forward to explain the RRATs, the newest subclass of neutron stars, and their connections to other radio pulsars. This work discusses these conjectures in the context of the characteristic properties of the RRAT population. Contrary to expectations, it is seen that - a) the RRAT population is statistically un-correlated with the nulling pulsars, and b) the RRAT phenomenon is unlikely to be related to old age or death-line proximity. It is perhaps more likely that the special emission property of RRATs is a signature of them being later evolutionary phases of other types of neutron stars which may have resulted in restructuring of the magnetic fields.
