中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Constraining the Orbital Inclination and Companion Properties of Three Black Widow Pulsars Detected by FAST

文献类型:期刊论文

作者Du, Ze-Xin1; Yu, Yun-Wei1,2; Chen, A-Ming3; Wang, Shuang-Qiang6; Zhou, Xia4,5,6; Zheng, Xiao-Ping1,2
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2023-12-01
卷号23期号:12页码:125024
关键词(stars:) binaries: eclipsing stars: winds outflows
ISSN号1674-4527
DOI10.1088/1674-4527/ad034b
产权排序4
英文摘要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.
WOS关键词MILLISECOND PULSAR ; PSR ; ECLIPSES ; EMISSION ; SHOCK ; STAR ; VARIABILITY ; EVOLUTION ; DISCOVERY
资助项目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研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001114804200001
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
资助机构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
源URL[http://ir.xao.ac.cn/handle/45760611-7/5640]  
专题脉冲星研究团组
通讯作者Yu, Yun-Wei
作者单位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.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China
5.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China
6.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
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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.

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