KMS of Xinjiang Astronomical Observatory, CAS
| Formation of long-period radio pulsars | |
Zhou, Xia1,2,3 ; Huang, Hai-Tao1,4; Cheng, Quan1,5; Zheng, Xiao-Ping5,6
| |
| 2024-04-13 | |
| Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| ISSN | 0035-8711 |
| Volume | 530Issue:2Pages:1636-1643 |
| Contribution Rank | 1 |
| Abstract | This study investigates the influence of different braking mechanisms on the formation of three long-period radio pulsars (PSRs J0250+5854, J2251-3711, and J0901-4046): plasma-filled magnetosphere in combination with magnetic field decay, fall-back disc, and r-mode instability. These braking mechanisms can also affect the thermal evolution of pulsars. By comparing the model-predicted values with observational data such as spin periods, period derivatives, and upper limits of the bolometric luminosity of these pulsars, we find that these three braking mechanisms can reasonably explain the spin period and the period derivative within a certain range of parameters for these sources. The model-predicted bolometric luminosity associated with magnetic field dissipation exceeds the upper limit for PSR J0901-4046 but falls below the upper limits for PSR J0250+5854 and PSR J2251-3711. The model-predicted bolometric luminosity within the fall-back disc model exceeds the observed results, whereas the luminosity within the r-mode instability falls below the observed upper limit for these three pulsars. However, a conflict arises when we consider the pulsar radio activity and the accretion phases within the fall-back disc model simultaneously. By combining data from radio and X-ray observations, along with precise measurements of surface thermal emissions, we can enhance our understanding of the braking mechanisms involved in the formation of long-period radio pulsars or constrain key model parameters. Finding more long-period pulsars in the future and conducting multiband observations will enhance our understanding of the formation and nature of long-period radio pulsars. |
| Keyword | pulsars: general pulsars: individual: PSR J0250+5854 pulsars: individual: PSR J2251-3711 pulsars: individual: PSR J0901-4046 stars: rotation |
| DOI | 10.1093/mnras/stae954 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | CENTRAL COMPACT OBJECTS ; X-RAY ; NEUTRON-STARS ; DEATH LINE ; SPIN-DOWN ; THERMAL EVOLUTION ; SNAPSHOT SURVEY ; MAGNETIC-FIELD ; INSTABILITY ; ACCRETION |
| Funding Project | National Natural Science Foundation of China[2021D04016] ; Opening Foundation of Xinjiang Key Laboratory[2023D01E20] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[12033001] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[12273028] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[12288102] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region[12003009] ; National Natural Science Foundation of China[2022YFC2205202] ; National Key R&D Program of China[2019-XBQNXZ-B-016] ; CAS 'Light of West China' Program[XJYWZ2303] ; Urumqi Nanshan Astronomy and Deep Space Exploration Observation and Research Station of Xinjiang |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001204006700005 |
| Publisher | OXFORD UNIV PRESS |
| Funding Organization | National Natural Science Foundation of China ; Opening Foundation of Xinjiang Key Laboratory ; Natural Science Foundation of Xinjiang Uygur Autonomous Region ; National Natural Science Foundation of China ; National Key R&D Program of China ; CAS 'Light of West China' Program ; Urumqi Nanshan Astronomy and Deep Space Exploration Observation and Research Station of Xinjiang |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6487 |
| Collection | 中国科学院新疆天文台 |
| Corresponding Author | Zhou, Xia |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 3.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China 4.Chongqing Inst Engn, Chongqing 400056, Peoples R China 5.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China 6.Huazhong Univ Sci & Technol, Sch Phys, Dept Astron, Wuhan 430074, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Zhou, Xia,Huang, Hai-Tao,Cheng, Quan,et al. Formation of long-period radio pulsars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,530(2):1636-1643. |
| APA | Zhou, Xia,Huang, Hai-Tao,Cheng, Quan,&Zheng, Xiao-Ping.(2024).Formation of long-period radio pulsars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,530(2),1636-1643. |
| MLA | Zhou, Xia,et al."Formation of long-period radio pulsars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 530.2(2024):1636-1643. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Zhou-2024-Formation （1518KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment