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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 Publication | ASTRONOMISCHE NACHRICHTEN
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ISSN | 0004-6337 |
Volume | 344Issue:1-2Pages:e20220111 |
Contribution Rank | 1 |
Abstract | The 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. |
Keyword | pulsar magnetic inclination angle braking index Nanshan 25-m Radio Telescope |
DOI | 10.1002/asna.20220111 |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | BRAKING INDEX ; RADIO PULSAR ; LIGHT CURVES ; X-RAY ; EVOLUTION ; EMISSION ; SPECTRA ; ALIGNMENT ; PROFILES ; GLITCHES |
Funding Project | Chinese National Science Foundation ; [12041304] |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000911530000001 |
Publisher | WILEY-V C H VERLAG GMBH |
Funding Organization | Chinese National Science Foundation |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://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 Author | Gao, Zhi-Fu |
Affiliation | 1.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 Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Corresponding Author Affilication | Xinjiang 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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