中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Revealing the Unseen: The Discovery of Long-awaited Radiation from the Intermittent Pulsar PSR B1931+24

文献类型:期刊论文

作者Rusul, Abdujappar5; Wen, Z. G.4; Yuan, J. P.4; Esamdin, Ali4; Zheng, X. P.3; Kramer, Michael1,2
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2026-03-01
卷号999期号:1页码:19
ISSN号2041-8205
DOI10.3847/2041-8213/ae3f2a
通讯作者Rusul, Abdujappar(aai-pulsar@qq.com)
英文摘要Pulsars are typically characterized by their stable, highly magnetized, and fast-rotating nature, which underpins their persistent radio emissions. However, the discovery of prolonged radio-quiet ("off") states in intermittent pulsars, such as PSR B1931+24, has been challenging the fundamental theory of pulsar magnetospheric emission. Despite long-term monitoring with several telescopes over 20 yr, the observations of PSR B1931+24 had not detected any significant emission during its "off" states. Recently, sensitive observations via the Five-hundred-meter Aperture Spherical radio Telescope revealed the mysterious weak emissions containing occasional faint bursting pulses during the "off" states of PSR B1931+24, signifying the theory of pulsar magnetospheric emission that the pulsar cannot remain off for long unless it truly dies. Along with a substantial decrease in flux density, a contraction and change in the integrated pulse profile are measured in the "off" state compared to the radio-loud ("on") state, indicating alterations in the plasma supply and magnetospheric structure. Additionally, previously unobserved asynchronous, nonuniform emission patterns are found in both states, implying a spatially inhomogeneous pair-cascade associated with the coherent radio emission of the pulsar. Furthermore, statistical comparisons between the faint off-state bursts and the on-state emission show that the faint bursts cannot be explained simply as a scaled-down version of the on-state emission. Instead, they constitute a distinct emission mode, plausibly linked to changes in plasma supply and the magnetospheric configuration of PSR B1931+24. These findings greatly advance our understanding of pulsar magnetospheric dynamics and emission mechanisms.
WOS关键词RADIO PULSAR ; SPIN-DOWN ; MAGNETOSPHERE ; SEARCHES ; ORIGIN ; NULLS ; MODEL ; GAPS
资助项目MOST divided by National Natural Science Foundation of China (NSFC)[12103021] ; Key Program of the National Natural Foundation of China[12033001] ; National SKA Program of China[2020SKA0120300] ; (sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic) divided by Natural Science Foundation of Xinjiang Uygur Autonomous Region (Xinjiang Natural Science Foundation)[2025D01A14]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001697528800001
出版者IOP Publishing Ltd
资助机构MOST divided by National Natural Science Foundation of China (NSFC) ; Key Program of the National Natural Foundation of China ; National SKA Program of China ; (sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic) divided by Natural Science Foundation of Xinjiang Uygur Autonomous Region (Xinjiang Natural Science Foundation)
源URL[http://ir.xao.ac.cn/handle/45760611-7/8602]  
专题脉冲星研究团组
通讯作者Rusul, Abdujappar
作者单位1.Max Planck Inst Radioastron, Bonn, Germany
2.Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Manchester, England
3.Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
5.Kashi Univ, Inst Phys & Elect Engn, Kashgar 844009, Peoples R China
推荐引用方式
GB/T 7714
Rusul, Abdujappar,Wen, Z. G.,Yuan, J. P.,et al. Revealing the Unseen: The Discovery of Long-awaited Radiation from the Intermittent Pulsar PSR B1931+24[J]. ASTROPHYSICAL JOURNAL LETTERS,2026,999(1):19.
APA Rusul, Abdujappar,Wen, Z. G.,Yuan, J. P.,Esamdin, Ali,Zheng, X. P.,&Kramer, Michael.(2026).Revealing the Unseen: The Discovery of Long-awaited Radiation from the Intermittent Pulsar PSR B1931+24.ASTROPHYSICAL JOURNAL LETTERS,999(1),19.
MLA Rusul, Abdujappar,et al."Revealing the Unseen: The Discovery of Long-awaited Radiation from the Intermittent Pulsar PSR B1931+24".ASTROPHYSICAL JOURNAL LETTERS 999.1(2026):19.

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