Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation
文献类型：期刊论文
| 作者 | Cui, Xiang-Han2,3; Zhang, Cheng-Min1,2,3; Li, Di2,3,4; Zhang, Jian-Wei2; Peng, Bo2,3,5; Zhu, Wei-Wei2,3,5; Strom, Richard6,7; Wang, Shuang-Qiang8 ; Wang, Na8; Wu, Qing-Dong8
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| 刊名 | Astrophysics and Space Science
 |
| 出版日期 | 2022-07-01 |
| 卷号 | 367期号:7页码:66 |
| ISSN号 | 0004-640X |
| 关键词 | Transients Fast radio burst methods Statistical stars Magnetars flare sgr-1806-20 pulsar Astronomy & Astrophysics |
| DOI | 10.1007/s10509-022-04093-y |
| 产权排序 | 8 |
| 文献子类 | Article |
| 英文摘要 | Fast radio bursts (FRBs) are extremely strong radio flares lasting several micro- to milliseconds and come from unidentified objects at cosmological distances, most of which are only seen once. Based on recently published data in the CHIME/FRB Catalog 1 in the frequency bands 400-800 MHz, we analyze 125 apparently singular FRBs with low dispersion measure (DM) and find that the distribution of their luminosity follows a lognormal form according to statistical tests. In our luminosity measurement, the FRB distance is estimated by using the Macquart relation that was obtained for 8 localized FRBs, and we find it still applicable for 18 sources after adding the latest 10 new localized FRBs. In addition, we test the validity of the luminosity distribution up to the Macquart relation and find that the lognormal-form feature decreases as the uncertainty increases. Moreover, we compare the luminosity of these apparent nonrepeaters with that of the previously observed 10 repeating FRBs also at low DM, noting that they belong to different lognormal distributions with the mean luminosity of nonrepeaters being two times greater than that of repeaters. Therefore, from the two different lognormal distributions, different mechanisms for FRBs can be implied. |
| URL标识 | 查看原文 |
| 语种 | 英语 |
| WOS记录号 | WOS:000821889300001 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/5130]  |
| 专题 | 星系宇宙学研究团组 |
| 作者单位 | 1.School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China; 2.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China; 3.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, China; 4.NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal, Durban 4000, South Africa; 5.Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Beijing 100101, China; 6.Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo, the Netherlands; 7.Astronomical Institute ‘Anton Pannekoek’, Faculty of Science, University of Amsterdam, 1090 GE Amsterdam, the Netherlands; 8.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, China; 9.School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550001, China; 10.School of Physics and Electronic Science, Guizhou Education University, Guiyang 550018, China |
| 推荐引用方式 GB/T 7714 | Cui, Xiang-Han,Zhang, Cheng-Min,Li, Di,et al. Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation[J]. Astrophysics and Space Science,2022,367(7):66. |
| APA | Cui, Xiang-Han.,Zhang, Cheng-Min.,Li, Di.,Zhang, Jian-Wei.,Peng, Bo.,...&Yang, Yi-Yan.(2022).Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation.Astrophysics and Space Science,367(7),66. |
| MLA | Cui, Xiang-Han,et al."Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation".Astrophysics and Space Science 367.7(2022):66. |
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