A Possible Kilonova Powered by Magnetic Wind from a Newborn Black Hole

A Possible Kilonova Powered by Magnetic Wind from a Newborn Black Hole
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可能由新生黑洞磁风驱动的千新星

DOI:
10.3847/1538-4357/abe71b
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发表时间:
2020-10
影响因子:
4.9
通讯作者:
Lei Wei-Hua
Lei Wei-Hua
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
Ma Shuai-Bing;Xie Wei;Liao Bin;Zhang Bin-Bin;Lu Hou-Jun;Liu Yu;Lei Wei-Hua

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The merger of binary neutron stars (NS–NS) as the progenitor of short gamma-ray bursts (GRBs) has been confirmed by the discovery of the association of the gravitational-wave (GW) event GW170817 with GRB 170817A. However, the merger product of binary NS r
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