Identifying disappearance of a white dwarf binary with LISA

被引：1
作者：
Seto, Naoki [1 ]
机构：
[1] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2023年 / 523卷 / 01期
关键词：
gravitational waves; binaries: close; MASS-TRANSFER; GRAVITATIONAL-WAVES; MERGER; EVOLUTION; SIMULATIONS; POPULATION; RESOLUTION; ONSET;
D O I：
10.1093/mnras/stad1420
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We discuss the prospect of identifying a white dwarf binary merger by monitoring disappearance of its nearly monochromatic gravitational wave. For a 10 yr operation of the laser interferometer space antenna (LISA), the chance probability of observing such an event is roughly estimated to be 20 per cent. By simply using short-term coherent signal integrations, we might determine the merger time with an accuracy of similar to 3-10 d. Also considering its expected sky localizability similar to 0.1-0.01 deg(2), LISA might make an interesting contribution to the multimessenger study on a merger event.
引用
收藏
页码：577 / 581
页数：5
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