一个低磁场柔软的玛反复器
1Institut de Ciéncies de l'Espai, Consejo Superior de Investigaciones Científicas, Institut d'Estudis Espacials de Catalunya, Facultat de Ciéncies, Campus UAB, Torre C5-parell, 2a planta, 08193 Bellaterra (Barcelona), Spain. rea@ieec.uab.es
概括
磁体,或由强烈的磁场驱动的中子星,可能不需要极高的表面场. 这项研究发现了一种柔软的玛反射器,具有类似磁器的爆发,但磁场较低,挑战了现有的理论.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 中子星物理学 中子星物理学
背景情况:
- 软玛重复器 (SGR) 和异常的X射线脉冲星是零星爆发的X射线源.
- 这些来源被假设是磁星,由极端磁场 (10^1410^15高斯) 提供动力.
研究的目的:
- 为了研究表现出磁器类活动的柔软玛反复器的磁场强度.
- 为了确定极高的磁场是否对磁器类行为至关重要.
主要方法:
- 软玛重复器SGR 0418+5729.9的X射线观测结果
- 对爆发辐射的分析,以推断磁场属性.
主要成果:
- SGR 0418+5729 呈现出类似磁星的爆发.
- X射线观测表明,二极磁场低于7.5 × 10^12高斯,这是无线电脉冲星的典型特征.
- 这表明磁星类活动可以发生在比以前假设的磁场更低的磁场中.
结论:
- 高表面双极磁场不是磁铁类活动的先决条件.
- 磁星群可能包含更广泛的磁场强度,年龄和进化状态的频谱.
- 这一发现扩大了我们对中子星多样性和磁星形成的理解.
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