Institutional Repository of Radio Astronomy Research Laboratory
| RRAT J1913+1330: An Extremely Variable and Puzzling Pulsar | |
Zhang, S. B.1; Geng, J. J.1; Wang, J. S.2; Yang, X.1,3; Kaczmarek, J.4,5; Tang, Z. F.1,3; Johnston, S.4; Hobbs, G.4; Manchester, R.4; Wu, X. F.1,3; Jiang, P.6,7; Huang, Y. F.8; Zou, Y. C.9; Dai, Z. G.10; Zhang, B.11; Li, D.6,12,13; Yang, Y. P.1,14; Dai, S.15; Chang, C. M.1,3; Pan, Z. C.6,7; Lu, J. G.6,7; Wei, J. J.1; Li, Y.1 ; Wu, Q. W.9; Qian, L.6,7; Wang, P.6,16; Wang, S. Q.17; Feng, Y.12; Staveley-Smith, L.18,19
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| 2024-09-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 972Issue:1Pages:59 |
| Contribution Rank | 17 |
| Abstract | Rotating radio transients (RRATs) are neutron stars that emit sporadic radio bursts. We detected 1955 single pulses from RRAT J1913+1330 using the 19 beam receiver of the Five-hundred-meter Aperture Spherical radio Telescope. These pulses were detected in 19 distinct clusters, with 49.4% of them occurring with a waiting time of one rotation period. The energy distribution of these individual pulses exhibited a wide range, spanning 3 orders of magnitude, reminiscent of repeating fast radio bursts (FRBs). Furthermore, we observed abrupt variations in pulse profile, width, peak flux, and fluence between adjacent sequential pulses. These findings suggest that this RRAT could be interpreted as a pulsar with extreme pulse-to-pulse modulation. The presence of sequential pulse trains during active phases, along with significant pulse variations in profile, fluence, flux, and width, should be intrinsic to a subset of RRATs. Our results indicate that J1913+1330 represents a peculiar source that shares certain properties with populations of nulling pulsars, giant pulses, and FRBs from different perspectives. The dramatic pulse-to-pulse variation observed in J1913+1330 could be attributed to unstable pair creation above the polar cap region and the variation of the site where streaming pairs emit coherently. Exploring a larger sample of RRATs exhibiting similar properties to J1913+1330 has the potential to significantly advance our understanding of pulsars, RRATs, and FRBs. |
| DOI | 10.3847/1538-4357/ad6602 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | ROTATING RADIO TRANSIENTS ; GIANT PULSES ; LONG-TERM ; POLARIZATION ; EMISSION ; SEARCHES ; I. |
| Funding Project | National SKA Program of China ; National Natural Science Foundation of China[12041306] ; National Natural Science Foundation of China[12003028] ; International Partnership Program of Chinese Academy of Sciences[114332KYSB20210018] ; National Key R&D Program of China[2021YFA0718500] ; China Postdoctoral Science Foundation[2020M681758] ; Natural Science Foundation of Jiangsu Province[BK20210998] ; Youth Innovation Promotion Association[2023331] ; Alexander von Humboldt Foundation ; Xinjiang Tianchi Program |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001297479100001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | National SKA Program of China ; National Natural Science Foundation of China ; International Partnership Program of Chinese Academy of Sciences ; National Key R&D Program of China ; China Postdoctoral Science Foundation ; Natural Science Foundation of Jiangsu Province ; Youth Innovation Promotion Association ; Alexander von Humboldt Foundation ; Xinjiang Tianchi Program |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6926 |
| 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 | Wu, X. F.; Jiang, P.; Dai, Z. G.; Zhang, B. |
| Affiliation | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China 2.Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany 3.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China 4.CSIRO Space & Astron, Epping, NSW 1710, Australia 5.Univ British Columbia, Dept Comp Sci Math Phys & Stat, Kelowna, BC V1V 1V7, Canada 6.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 7.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing 100101, Peoples R China 8.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China 9.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Peoples R China 10.Univ Sci & Technol China, Dept Astron, Hefei 230026, Peoples R China 11.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA 12.Res Ctr Intelligent Comp Platforms, Zhejiang Lab, Hangzhou 311100, Peoples R China 13.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 14.Yunnan Univ, South Western Inst Astron Res, Kunming 650504, Peoples R China 15.Western Sydney Univ, Sch Sci, Locked Bag 1797, Penrith, NSW 2751, Australia 16.Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China 17.Chinese Acad Sci, Xinjiang Astron Observ, Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 18.Univ Western Australia, Int Ctr Radio Astron Res, Crawley, WA 6009, Australia 19.ARC Ctr Excellence All Sky Astrophys 3 Dimens ASTR, Canberra, Australia |
| Recommended Citation GB/T 7714 | Zhang, S. B.,Geng, J. J.,Wang, J. S.,et al. RRAT J1913+1330: An Extremely Variable and Puzzling Pulsar[J]. ASTROPHYSICAL JOURNAL,2024,972(1):59. |
| APA | Zhang, S. B..,Geng, J. J..,Wang, J. S..,Yang, X..,Kaczmarek, J..,...&Staveley-Smith, L..(2024).RRAT J1913+1330: An Extremely Variable and Puzzling Pulsar.ASTROPHYSICAL JOURNAL,972(1),59. |
| MLA | Zhang, S. B.,et al."RRAT J1913+1330: An Extremely Variable and Puzzling Pulsar".ASTROPHYSICAL JOURNAL 972.1(2024):59. |
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| Zhang-2024-RRAT J191（1411KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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