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首页> 外文期刊>Chinese Journal of Astronomy and Astrophysics >Short-living Supermassive Magnetar Model for the Early X-ray Flares Following Short GRBs
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Short-living Supermassive Magnetar Model for the Early X-ray Flares Following Short GRBs

机译:短GRB之后的早期X射线耀斑的短生命超大规模磁模型

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摘要

We suggest a short-lived supermassive magnetar model to account for the X-ray flares following short γ-ray bursts. In this model the central engine of the short γ-ray bursts is a supermassive millisecond magnetar, formed in coalescence of double neutron stars. The X-ray flares are powered by the dipole radiation of the magnetar. When the magnetar has lost a significant part of its angular momentum, it collapses to a black hole and the X-ray flares cease abruptly.
机译:我们建议使用短寿命的超大质量电磁模型来解释短时间γ射线爆发后的X射线耀斑。在该模型中,短γ射线爆发的中心引擎是一个超大质量的毫秒磁石,由双中子星的聚结形成。 X射线耀斑由磁星的偶极辐射提供动力。当磁星失去大部分角动量时,它会坍塌成一个黑洞,并且X射线耀斑突然停止。

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