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机译:球形簇光度函数距离至NGC 4993托管二元中子星形合并GW170817 / GRB 170817A
Astronomy Program Department of Physics and Astronomy Seoul National University Gwanak-gu Seoul 08826 Republic of Korea;
Astronomy Program Department of Physics and Astronomy Seoul National University Gwanak-gu Seoul 08826 Republic of Korea;
Astronomy Program Department of Physics and Astronomy Seoul National University Gwanak-gu Seoul 08826 Republic of Korea;
galaxies: distances and redshifts; galaxies: elliptical and lenticular; cD; galaxies: individual (NGC 4993); galaxies: star clusters: general; gravitational waves;
机译:球形簇光度函数距离至NGC 4993托管二元中子星形合并GW170817 / GRB 170817A
机译:来自二进制中子星合并的引力波和伽马射线:GW170817和GRB 170817A
机译:使用表面亮度波动的二元中子星形合并GW170817的主机星系的精确距离
机译:第一个双星中子星GW 170817 / GRB 170817A与Giant Metrewave射电望远镜的低频观察
机译:紧凑的物体自旋对寻找来自双星中子星和中子星-黑洞合并的引力波的影响。
机译:双中子星合并祖先产生的特殊低发光度短伽马射线爆发
机译:球形簇亮度函数距离到NGC 4993托管二进制中子星合并GW170817 / GRB 170817A