| Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries, and gravitational wave sources | |
Chen HL(陈海亮)1,2,3 ; Tauris, Thomas M.3,4; Han ZW(韩占文)1,2,5,6; Chen XF(陈雪飞)1,2,5,6
| |
| 发表期刊 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 2021-03-31 | |
| 卷号 | 503期号:3页码:3540-3551 |
| DOI | 10.1093/mnras/stab670 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI ; EI |
| 关键词 | gravitational waves binaries: close stars: neutron pulsars: general white dwarfs X-rays: binaries |
| 摘要 | Close-orbit low-mass X-ray binaries (LMXBs), radio binary millisecond pulsars (BMSPs) with extremely low-mass helium white dwarfs (ELM He WDs) and ultra-compact X-ray binaries (UCXBs) are all part of the same evolutionary sequence. It is therefore of uttermost importance to understand how these populations evolve from one specie to another. Moreover, UCXBs are important gravitational wave (GW) sources and can be detected by future space-borne GW observatories. However, the formation and evolutionary link between these three different populations of neutron star (NS) binaries are not fully understood. In particular, a peculiar fine-tuning problem has previously been demonstrated for the formation of these systems. In this investigation, we test a newly suggested magnetic braking prescription and model the formation and evolution of LMXBs. We compute a grid of binary evolution models and present the initial parameter space of the progenitor binaries which successfully evolve all the way to produce UCXBs. We find that the initial orbital period range of LMXBs, which evolve into detached NS + ELM He WD binaries and later UCXBs, becomes significantly wider compared to evolution with a standard magnetic braking prescription, and thus helps to relieve the fine-tuning problem. However, we also find that formation of wide-orbit BMSPs is prohibited for strong versions of this new magnetic braking prescription, which therefore calls for a revision of the prescription. Finally, we present examples of the properties of UCXBs as Galactic GW sources and discuss their detection by the LISA, TianQin, and Taiji observatories. |
| 资助项目 | Aarhus University ; National Natural Science Foundation of China[12090040] ; National Natural Science Foundation of China[12090043] ; National Natural Science Foundation of China[11521303] ; National Natural Science Foundation of China[12073071] ; National Natural Science Foundation of China[11873016] ; National Natural Science Foundation of China[11733008] ; Yunnan Province[202001AT070058] ; CAS light of West China Program, Youth Innovation Promotion Association, Chinese Academy of Sciences[2018076] ; European Union's Horizon 2020 Research and Innovation Programme[754513] ; Aarhus University Research Foundation |
| 项目资助者 | Aarhus University ; National Natural Science Foundation of China[12090040, 12090043, 11521303, 12073071, 11873016], 11733008] ; Yunnan Province[202001AT070058] ; CAS light of West China Program, Youth Innovation Promotion Association, Chinese Academy of Sciences[2018076] ; European Union's Horizon 2020 Research and Innovation Programme[754513] ; Aarhus University Research Foundation |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 恒星与银河系 ; 恒星形成与演化 |
| 文章类型 | Article |
| 出版者 | OXFORD UNIV PRESS |
| 出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
| ISSN | 0035-8711 |
| URL | 查看原文 |
| WOS记录号 | WOS:000770093700027 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | REDUCED MAGNETIC BRAKING ; ROTATING MASSIVE STARS ; PRESUPERNOVA EVOLUTION ; CONVECTIVE BOUNDARIES ; STELLAR EVOLUTION ; MODULES ; SYSTEMS ; PERIOD |
| EI入藏号 | 20221712023692 |
| EI主题词 | Gravity waves |
| EI分类号 | 657.2 Extraterrestrial Physics and Stellar Phenomena - 701.2 Magnetism: Basic Concepts and Phenomena - 804 Chemical Products Generally - 931.5 Gravitation, Relativity and String Theory |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/24405 |
| 专题 | 大样本恒星演化研究组 中国科学院天体结构与演化重点实验室 |
| 通讯作者 | Chen HL(陈海亮); Chen XF(陈雪飞) |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China 3.Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark 4.Aarhus Institute of Advanced Studies (AIAS), Aarhus University, Høegh-Guldbergs Gade 6B, DK-8000 Aarhus C, Denmark 5.University of the Chinese Academy of Sciences, Yuquan Road 19, Shijingshan Block, Beijing 100049, China 6.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China |
| 第一作者单位 | 中国科学院云南天文台 |
| 通讯作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Chen HL,Tauris, Thomas M.,Han ZW,et al. Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries, and gravitational wave sources[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,503(3):3540-3551. |
| APA | Chen HL,Tauris, Thomas M.,Han ZW,&Chen XF.(2021).Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries, and gravitational wave sources.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,503(3),3540-3551. |
| MLA | Chen HL,et al."Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries, and gravitational wave sources".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 503.3(2021):3540-3551. |
| 条目包含的文件 | ||||||
| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| Formation of millise（1093KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。
修改评论