机译:从Macronova观察中断中子星黑洞聚结率
Chinese Acad Sci Purple Mt Observ Key Lab Dark Matter &
Space Astron Nanjing 210008 Jiangsu Peoples R China;
Sun Yat Sen Univ TianQin Res Ctr Gravitat Phys Zhuhai 519082 Peoples R China;
Chinese Acad Sci Purple Mt Observ Key Lab Dark Matter &
Space Astron Nanjing 210008 Jiangsu Peoples R China;
Chinese Acad Sci Purple Mt Observ Key Lab Dark Matter &
Space Astron Nanjing 210008 Jiangsu Peoples R China;
Chinese Acad Sci Purple Mt Observ Key Lab Dark Matter &
Space Astron Nanjing 210008 Jiangsu Peoples R China;
gravitational waves; stars: black holes; stars: neutron;
机译:从Macronova观察中断中子星黑洞聚结率
机译:核合成受中子星黑孔合并速率的约束
机译:用中子星-黑洞聚结二元的引力波和短伽马射线爆裂联合观测来约束中子星半径
机译:GRB 060614中的R-Process Macronova / kilonova:中子星黑洞二进制文件合并的证据
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:黑洞-中子星双星的合并
机译:凝聚中子星-黑洞双星的最内层稳定圆形轨道:广义伪牛顿势能法