中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
New Potential Ultracompact X-Ray Binaries for Space-based Gravitational-wave Detectors from a Low-mass Main-sequence Companion Channel

文献类型:期刊论文

作者Chen, Minghua1,2; Liu, Jinzhong1,2
刊名ASTROPHYSICAL JOURNAL
出版日期2025-03-10
卷号981期号:2页码:175
ISSN号0004-637X
DOI10.3847/1538-4357/adb618
产权排序1
英文摘要We investigate the formation and evolution of ultracompact X-ray binaries (UCXBs) using the COMPAS binary evolution code, starting from the zero-age main sequence (MS). Focusing on the low-mass MS companion channel, we simulate gravitational-wave (GW) signals from UCXBs with LEGWORK and evaluate their detectability by space-based observatories such as Taiji and TianQin. By incorporating signal-to-noise ratio (SNR) calculations with a threshold of SNR > 5, we provide a realistic framework to assess the detectability of the GW source. Our analysis suggests that the Milky Way currently hosts 7-32 observable UCXBs from the MS companion channel. Taiji or LISA alone could detect one to six sources over an 8 yr observation period, while TianQin, due to its high-frequency sensitivity, contributes to detecting systems with extremely short orbital periods and can also detect one to four sources. Comparison with sensitivity curves validates UCXBs as detectable GW sources, particularly at greater Galactic distances. This study improves our understanding of the evolution of UCXBs and their role as GW sources. By integrating population synthesis, SNR-based analyses, and observational data, we establish UCXBs as significant targets for GW astronomy, paving the way for future missions and theoretical studies of compact binary systems.
WOS关键词ACCRETION-INDUCED COLLAPSE ; ULTRA-COMPACT BINARIES ; HELIUM WHITE-DWARFS ; MILLISECOND PULSAR ; GLOBULAR-CLUSTERS ; ORBITAL PERIOD ; EVOLUTION ; STAR ; STELLAR ; DISCOVERY
资助项目Tianshan Talent Training Program ; Central Guidance for Local Science and Technology Development Fund[ZYYD2025QY27] ; National Natural Science Foundation of China NSFC[12433007] ; China Manned Space Project[CMS-CSST-2021-A08] ; [2023TSYCCX0101]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001439716500001
出版者IOP Publishing Ltd
资助机构Tianshan Talent Training Program ; Central Guidance for Local Science and Technology Development Fund ; National Natural Science Foundation of China NSFC ; China Manned Space Project
源URL[http://ir.xao.ac.cn/handle/45760611-7/7484]  
专题光学天文与技术应用研究室_变星研究团组
通讯作者Liu, Jinzhong
作者单位1.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
推荐引用方式
GB/T 7714
Chen, Minghua,Liu, Jinzhong. New Potential Ultracompact X-Ray Binaries for Space-based Gravitational-wave Detectors from a Low-mass Main-sequence Companion Channel[J]. ASTROPHYSICAL JOURNAL,2025,981(2):175.
APA Chen, Minghua,&Liu, Jinzhong.(2025).New Potential Ultracompact X-Ray Binaries for Space-based Gravitational-wave Detectors from a Low-mass Main-sequence Companion Channel.ASTROPHYSICAL JOURNAL,981(2),175.
MLA Chen, Minghua,et al."New Potential Ultracompact X-Ray Binaries for Space-based Gravitational-wave Detectors from a Low-mass Main-sequence Companion Channel".ASTROPHYSICAL JOURNAL 981.2(2025):175.

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