arXiv 0801.13652008-01-09astro-ph

磁星的形成：孤立之谜

Formation Scenario of Magnetars: The Puzzle of Isolation

Nirvikar Prasad

备注：: Prepared for the conference "40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More", August 12-17, 2007, McGill University, Montreal, Canada

摘要：

磁星（SGR和AXP）是中子星演化的重要途径之一。这些天体在其表面有一个超强磁场$B \sim 10^{15}$ G，并显示出持续的X射线脉动和瞬时爆发。到目前为止，已知有14颗磁星：5颗SGR（4颗确认，1颗候选）和9颗AXP（7颗确认，2颗候选）。这是一个开放的难题，所有这些对象是孤立的，没有发现在二进制。我们将讨论可能导致这种情况的形成方案。

英文摘要：

Magnetars (SGRs and AXPs) are one of the most evolutionary paths of a neutron star. These objects have an ultra-strong magnetic field $B \sim 10^{15}$ G at their surface and show persistent X-ray pulsations and transient bursts. Till date there are 14 magnetars known: 5 SGRs (4 confirmed, 1 candidate) and 9 AXPs (7 confirmed, 2 candidates). It is an open puzzle that all these objects are isolated and none have been found in binaries. We discuss the formation scenario which can lead to such a situation.

机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。