Institutional Repository of Radio Astronomy Research Laboratory
| Constraining the Orbital Inclination and Companion Properties of Three Black Widow Pulsars Detected by FAST | |
Du, Ze-Xin1; Yu, Yun-Wei1,2; Chen, A-Ming3; Wang, Shuang-Qiang4 ; Zhou, Xia4,5,6; Zheng, Xiao-Ping1,2
| |
| 2023-12-01 | |
| Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
 |
| ISSN | 1674-4527 |
| Volume | 23Issue:12Pages:125024 |
| Contribution Rank | 4 |
| Abstract | Black widows (BWs) are millisecond pulsars ablating their companion stars. The out-flowing material from the companion can block the radio emission of the pulsar, resulting in eclipses. In this paper, we construct a model for the radio eclipse by calculating the geometry of the bow shock between the winds of the pulsar and companion, where the shock shapes the eclipsing medium but had not been described in detail in previous works. The model is further used to explain the variations of the flux density and dispersion measure of three BW pulsars (i.e., PSR B1957+20, J2055+3829, and J2051-0827) detected by the Five-hundred-meter Aperture Spherical radio Telescope. Consequently, we constrained the parameters of the three BW systems such as the inclination angles and true anomalies of the observer as well as the mass-loss rates and wind velocity of the companion stars. With the help of these constraints, it is expected that magnetic fields of companion stars and even masses of pulsars could further be determined as some extra observation can be achieved in the future. |
| Keyword | (stars:) binaries: eclipsing stars: winds outflows |
| DOI | 10.1088/1674-4527/ad034b |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | MILLISECOND PULSAR ; PSR ; ECLIPSES ; EMISSION ; SHOCK ; STAR ; VARIABILITY ; EVOLUTION ; DISCOVERY |
| Funding Project | National SKA program of China[2020SKA0120300] ; National Key R&D Program of China[2021YFA0718500] ; National Natural Science Foundation of China[11833003] ; National Natural Science Foundation of China[12033001] ; China Postdoctoral Science Foundation[2023T160410] ; Opening Foundation of Xinjiang Key Laboratory[2021D04016] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001114804200001 |
| Publisher | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
| Funding Organization | National SKA program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; China Postdoctoral Science Foundation ; Opening Foundation of Xinjiang Key Laboratory |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5641 |
| Collection | 射电天文研究室_脉冲星研究团组 |
| Corresponding Author | Yu, Yun-Wei |
| Affiliation | 1.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China 2.Cent China Normal Univ, Key Lab Quark & Lepton Phys, Minist Educ, Wuhan 430079, Peoples R China 3.Shanghai Jiao Tong Univ, Tsung Dao Lee Inst, Shanghai 201210, Peoples R China 4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 5.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 6.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China |
| Recommended Citation GB/T 7714 | Du, Ze-Xin,Yu, Yun-Wei,Chen, A-Ming,et al. Constraining the Orbital Inclination and Companion Properties of Three Black Widow Pulsars Detected by FAST[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2023,23(12):125024. |
| APA | Du, Ze-Xin,Yu, Yun-Wei,Chen, A-Ming,Wang, Shuang-Qiang,Zhou, Xia,&Zheng, Xiao-Ping.(2023).Constraining the Orbital Inclination and Companion Properties of Three Black Widow Pulsars Detected by FAST.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,23(12),125024. |
| MLA | Du, Ze-Xin,et al."Constraining the Orbital Inclination and Companion Properties of Three Black Widow Pulsars Detected by FAST".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 23.12(2023):125024. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Du-2023-Constraining（882KB） | 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