论文标题
引力波和短伽马射线爆发GW170817/SHB170817A，不是您的日常二进制中子星星合并
The gravitational wave and short gamma-ray burst GW170817/SHB170817A, not your everyday binary neutron star merger
论文作者
论文摘要
到目前为止，这一事件是独特的，完美地证实了由两个中子星的合并产生的引力波的标准视图，但其电磁多速度的观察结果与伽马射线爆发的“标准火球模型”的众多初始版本不同意。相反，他们提供了有力的证据，以支持“炮弹”模型。最毫无争议的是，在无线电波长处观察到一个炮弹，具有压倒性的统计意义（$> \！17 \，σ$），并在预期的情况下乘坐天空飞机乘坐明显的高光速度$ v_ {app} {app} \ sim 4 \，c $。
This event, so far unique, beautifully confirmed the standard views on the gravitational waves produced by a merger of two neutron stars, but its electromagnetic multi-wavelenth observations disagreed with the numerous initial versions of the "standard fireball model(s)" of gamma ray bursts. Contrariwise, they provided strong evidence in favour of the "cannonball" model. Most uncontroversially, a cannonball was observed at radio wavelengths, with an overwhelming statistical significance ($>\! 17\,σ$), and travelling in the plane of the sky, as expected, at an apparent superluminal velocity $V_{app}\sim 4\, c$.
