Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars?
文献类型:期刊论文
作者 | Chen HL(陈海亮)1,2,5; Tauris, Thomas M.4; Chen XF(陈雪飞)1,2,3,5; Han ZW(韩占文)1,2,3,5 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2023-07-01 |
卷号 | 951期号:2 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/acd4b8 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | The formation path to ultracompact X-ray binaries (UCXBs) with black hole (BH) accretors is still unclear. In the classical formation scenario, it is difficult to eject the massive envelope of the progenitor star of the BH via the common envelope process. Given that some neutron stars (NSs) in binary systems evidently have birth masses close to & SIM;2.0 M (& ODOT;), we explore here the possibility that BH-UCXBs may form via the accretion-induced collapse (AIC) of accreting NSs, assuming that these previously evolved in low-mass X-ray binaries to masses all the way up to the maximum limit of an NS. We demonstrate this formation path by modeling a few cases of NS-UCXBs with initial NS masses close to the maximum mass of an NS that evolve into BH-UCXBs after the NS accretes material from its He white dwarf (WD) companion. We follow the evolution of the post-AIC BH-UCXB and, based on simple arguments, we anticipate that there is about one BH-UCXB with an AIC origin and a He WD donor within the current sample of known UCXBs and that two to five such BH-UCXBs may be detected in gravitational waves by LISA. In addition, we find that the X-ray luminosity of NS-UCXBs near their orbital period minimum exceeds & SIM;10(39) erg s(-1), and thus, such systems may appear as ultraluminous X-ray sources. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星形成与演化 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | MAXIMUM MASS ; WHITE-DWARFS ; MILLISECOND PULSARS ; CONVECTIVE BOUNDARIES ; DONOR STARS ; EVOLUTION ; ASTROPHYSICS ; MODULES ; CONSTRAINTS ; EXPLOSIONS |
资助项目 | National Key Ramp ; D Program of China[2021YFA1600403] ; National Key Ramp ; D Program of China[2021YFA1600401] ; National Natural Science Foundation of China[12090040/12090043] ; National Natural Science Foundation of China[12073071] ; National Natural Science Foundation of China[11873016] ; National Natural Science Foundation of China[11733008] ; National Natural Science Foundation of China[12125303] ; Yunnan Fundamental Research Projects[202001AT070058] ; Yunnan Fundamental Research Projects[202101AW070003] ; Yunnan Fundamental Research Projects[202201BC070003] ; China Manned Space Project[202305AB350003] ; CAS Light of West China Program ; Yunnan Revitalization Talent Support Program-Science Technology Champion Project ; [CMS-CSST-2021-A10] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP Publishing Ltd |
WOS记录号 | WOS:001022709500001 |
资助机构 | National Key Ramp ; D Program of China[2021YFA1600403, 2021YFA1600401] ; National Natural Science Foundation of China[12090040/12090043, 12073071, 11873016, 11733008, 12125303] ; Yunnan Fundamental Research Projects[202001AT070058, 202101AW070003, 202201BC070003] ; China Manned Space Project[202305AB350003] ; CAS Light of West China Program ; Yunnan Revitalization Talent Support Program-Science Technology Champion Project ; [CMS-CSST-2021-A10] |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/26136] |
专题 | 云南天文台_大样本恒星演化研究组 云南天文台_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) |
作者单位 | 1.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, People's Republic of China; 2.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China; 3.University of the Chinese Academy of Sciences, Yuquan Road 19, Shijingshan Block, Beijing 100049, People's Republic of China 4.Department of Materials and Production, Aalborg University, Skjernvej 4A, DK-9220 Aalborg Øst, Denmark; 5.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People's Republic of China; chenhl@ynao.ac.cn; |
推荐引用方式 GB/T 7714 | Chen HL,Tauris, Thomas M.,Chen XF,et al. Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars?[J]. ASTROPHYSICAL JOURNAL,2023,951(2). |
APA | Chen HL,Tauris, Thomas M.,Chen XF,&Han ZW.(2023).Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars?.ASTROPHYSICAL JOURNAL,951(2). |
MLA | Chen HL,et al."Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars?".ASTROPHYSICAL JOURNAL 951.2(2023). |
入库方式: OAI收割
来源:云南天文台
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