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Burst timescales and luminosities as links between young pulsars and fast radio bursts
文献类型：期刊论文
| 作者 | Nimmo, K.28,29; Hessels, J. W. T.28,29; Kirsten, F.27,29; Keimpema, A.26; Cordes, J. M.24,25; Snelders, M. P.28; Hewitt, D. M.28; Karuppusamy, R.23; Archibald, A. M.12,22; Bezrukovs, V.21 |
| 刊名 | NATURE ASTRONOMY
 |
| 出版日期 | 2022-02-23 |
| 页码 | 17 |
| ISSN号 | 2397-3366 |
| DOI | 10.1038/s41550-021-01569-9 |
| 通讯作者 | Nimmo, K.(k.nimmo@uva.nl) |
| 英文摘要 | The range of timescales and luminosities measured from the nearby fast radio burst FRB 20200120E observationally connects these extreme extragalactic transients with studies of Galactic neutron stars. Fast radio bursts (FRBs) are extragalactic radio flashes of unknown physical origin. Their high luminosities and short durations require extreme energy densities, such as those found in the vicinity of neutron stars and black holes. Studying the burst intensities and polarimetric properties on a wide range of timescales, from milliseconds down to nanoseconds, is key to understanding the emission mechanism. However, high-time-resolution studies of FRBs are limited by their unpredictable activity levels, available instrumentation and temporal broadening in the intervening ionized medium. Here we show that the repeating FRB 20200120E can produce isolated shots of emission as short as about 60 nanoseconds in duration, with brightness temperatures as high as 3 x 10(41) K (excluding relativistic effects), comparable with 'nano-shots' from the Crab pulsar. Comparing both the range of timescales and luminosities, we find that FRB 20200120E observationally bridges the gap between known Galactic young pulsars and magnetars and the much more distant extragalactic FRBs. This suggests a common magnetically powered emission mechanism spanning many orders of magnitude in timescale and luminosity. In this Article, we probe a relatively unexplored region of the short-duration transient phase space; we highlight that there probably exists a population of ultrafast radio transients at nanosecond to microsecond timescales, which current FRB searches are insensitive to. |
| WOS关键词 | POLARIZATION ; EMISSION ; STATISTICS ; CLASSIFIER ; UNIVERSE ; PULSES |
| 资助项目 | EVN project[EK048] ; European Union's Horizon 2020 research and innovation programme[730562] ; European Union's Horizon 2020 research and innovation programme[101004719] ; Spanish Ministerio de Economia y Competitividad[AYA2016-76012-C3-1-P] ; Spanish Ministerio de Ciencia e Innovacion of the Institut de Ciencies del Cosmos of the Universitat de Barcelona (Unidad de Excelencia 'Maria de Maeztu' 2020-2023)[PID2019-105510GB-C31] ; Spanish Ministerio de Ciencia e Innovacion of the Institut de Ciencies del Cosmos of the Universitat de Barcelona (Unidad de Excelencia 'Maria de Maeztu' 2020-2023)[CEX2019-000918-M] ; US Department of Defense through the National Defense Science & Engineering Graduate Fellowship Program ; Dutch Research Council (NWO) Veni Fellowship ; Swedish Research Council ; Natural Sciences and Engineering Research Council of Canada ; Canadian Institute for Advanced Research ; National Program on Key Research and Development Project[2017YFA0402602] ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation[2008031] ; FRQNT Doctoral Research Award ; National Natural Science Foundation of China[12041304] ; National Natural Science Foundation of China[11873080] ; Dunlap Institute ; Engineering Research Institute Ventspils International Radio Astronomy Centre ; NWO Vici grant[VI.C.192.045] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | NATURE PORTFOLIO |
| WOS记录号 | WOS:000760082600001 |
| 资助机构 | EVN project ; European Union's Horizon 2020 research and innovation programme ; Spanish Ministerio de Economia y Competitividad ; Spanish Ministerio de Ciencia e Innovacion of the Institut de Ciencies del Cosmos of the Universitat de Barcelona (Unidad de Excelencia 'Maria de Maeztu' 2020-2023) ; US Department of Defense through the National Defense Science & Engineering Graduate Fellowship Program ; Dutch Research Council (NWO) Veni Fellowship ; Swedish Research Council ; Natural Sciences and Engineering Research Council of Canada ; Canadian Institute for Advanced Research ; National Program on Key Research and Development Project ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation ; FRQNT Doctoral Research Award ; National Natural Science Foundation of China ; Dunlap Institute ; Engineering Research Institute Ventspils International Radio Astronomy Centre ; NWO Vici grant |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/4504]  |
| 专题 | 脉冲星研究团组 射电天文研究室_利用南山26米射电望远镜观测数据的文章 |
| 通讯作者 | Nimmo, K. |
| 作者单位 | 1.Sidrat Res, Toronto, ON, Canada 2.Xinjiang Astron Observ, Urumqi, Peoples R China 3.Natl Ctr Radio Astrophys, Pune, Maharashtra, India 4.Tata Inst Fundamental Res, Dept Astron & Astrophys, Mumbai, Maharashtra, India 5.Univ British Columbia, Dept Phys & Astron, Vancouver, BC, Canada 6.Perimeter Inst Theoret Phys, Waterloo, ON, Canada 7.CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA 8.MIT, Dept Phys, Cambridge, MA 02139 USA 9.MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA 10.Russian Acad Sci, Inst Appl Astron, St Petersburg, Russia |
| 推荐引用方式 GB/T 7714 | Nimmo, K.,Hessels, J. W. T.,Kirsten, F.,et al. Burst timescales and luminosities as links between young pulsars and fast radio bursts[J]. NATURE ASTRONOMY,2022:17. |
| APA | Nimmo, K..,Hessels, J. W. T..,Kirsten, F..,Keimpema, A..,Cordes, J. M..,...&Yuan, J. P..(2022).Burst timescales and luminosities as links between young pulsars and fast radio bursts.NATURE ASTRONOMY,17. |
| MLA | Nimmo, K.,et al."Burst timescales and luminosities as links between young pulsars and fast radio bursts".NATURE ASTRONOMY (2022):17. |
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