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A short review on the pulsar magnetic inclination angles
Li, Biao-Peng1,2,3; Gao, Zhi-Fu1,2,4
2023-01-05
Source PublicationASTRONOMISCHE NACHRICHTEN
ISSN0004-6337
Volume344Issue:1-2Pages:e20220111
Contribution Rank1
AbstractThe inclination angle chi between the magnetic and rotation axes of pulsars is an important parameter in pulsar physics. The changes in the inclination angle of a pulsar would lead to observable effects, such as changes in the pulse beam width and braking index of the star. In this paper, we perform a short review on the evolution of a pulsar's magnetic inclination angle, as well as the latest research progress. Using an alignment rotator model in a vacuum, we investigate the magnetic inclination angle change rates for 12 high-braking index pulsars without a glitch, whose timing observations are obtained using the Nanshan 25-m Radio Telescope at Xinjiang Astronomical Observatory. For our purpose, three representative pulsars J0157+6212, J1743-3150, and J1857+0526 are chosen and their rotation and inclination angle evolutions are further investigated. In the future, radio and x-ray polarimetric observations will provide more information about the inclination angles of pulsars, which could help us understand the origin of the variations in chi of pulsars and shed light on the range of possibilities of pulsar magnetic field configuration. A continuous study of the pulsar inclination angle will provide an important window into additional physical processes at work in the young and highly magnetized pulsars.
Keywordpulsar magnetic inclination angle braking index Nanshan 25-m Radio Telescope
DOI10.1002/asna.20220111
Indexed BySCI
Language英语
WOS KeywordBRAKING INDEX ; RADIO PULSAR ; LIGHT CURVES ; X-RAY ; EVOLUTION ; EMISSION ; SPECTRA ; ALIGNMENT ; PROFILES ; GLITCHES
Funding ProjectChinese National Science Foundation ; [12041304]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000911530000001
PublisherWILEY-V C H VERLAG GMBH
Funding OrganizationChinese National Science Foundation
Citation statistics
Cited Times:17[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5042
Collection射电天文研究室_脉冲星研究团组
科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章
Corresponding AuthorGao, Zhi-Fu
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing, Peoples R China
3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1-St, Urumqi 830011, Xinjiang, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Li, Biao-Peng,Gao, Zhi-Fu. A short review on the pulsar magnetic inclination angles[J]. ASTRONOMISCHE NACHRICHTEN,2023,344(1-2):e20220111.
APA Li, Biao-Peng,&Gao, Zhi-Fu.(2023).A short review on the pulsar magnetic inclination angles.ASTRONOMISCHE NACHRICHTEN,344(1-2),e20220111.
MLA Li, Biao-Peng,et al."A short review on the pulsar magnetic inclination angles".ASTRONOMISCHE NACHRICHTEN 344.1-2(2023):e20220111.
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