Fast radio bursts at the dawn of the 2020s

IF 27.8 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
E. Petroff, J. W. T. Hessels, D. R. Lorimer
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引用次数: 69

Abstract

Since the discovery of the first fast radio burst (FRB) in 2007, and their confirmation as an abundant extragalactic population in 2013, the study of these sources has expanded at an incredible rate. In our 2019 review on the subject, we presented a growing, but still mysterious, population of FRBs—60 unique sources, 2 repeating FRBs, and only 1 identified host galaxy. However, in only a few short years, new observations and discoveries have given us a wealth of information about these sources. The total FRB population now stands at over 600 published sources, 24 repeaters, and 19 host galaxies. Higher time resolution data, sustained monitoring, and precision localisations have given us insight into repeaters, host galaxies, burst morphology, source activity, progenitor models, and the use of FRBs as cosmological probes. The recent detection of a bright FRB-like burst from the Galactic magnetar SGR 1935 + 2154 provides an important link between FRBs and magnetars. There also continue to be surprising discoveries, like periodic modulation of activity from repeaters and the localisation of one FRB source to a relatively nearby globular cluster associated with the M81 galaxy. In this review, we summarise the exciting observational results from the past few years. We also highlight their impact on our understanding of the FRB population and proposed progenitor models. We build on the introduction to FRBs in our earlier review, update our readers on recent results, and discuss interesting avenues for exploration as the field enters a new regime where hundreds to thousands of new FRBs will be discovered and reported each year.

本世纪20年代初的快速射电暴
自从2007年发现第一个快速射电暴(FRB),并在2013年证实它们是丰富的河外人口以来,对这些来源的研究以令人难以置信的速度扩展。在我们2019年对该主题的回顾中,我们提出了一个不断增长但仍然神秘的快速射电暴种群——60个独特的来源,2个重复的快速射电暴,只有1个确定的宿主星系。然而,在短短几年内,新的观察和发现给了我们关于这些来源的丰富信息。目前,快速射电暴总数超过600个已公布的源,24个中继器和19个宿主星系。更高的时间分辨率数据,持续的监测和精确的定位使我们能够深入了解中继器,宿主星系,爆发形态,源活动,祖模型,以及使用快速射电暴作为宇宙探测器。最近从银河系磁星SGR 1935 + 2154探测到一个明亮的类似快速射电暴的爆发,这为快速射电暴和磁星之间提供了一个重要的联系。还有一些令人惊讶的发现,比如中继器活动的周期性调制,以及一个快速射电暴源定位于相对较近的与M81星系相关的球状星团。在这篇综述中,我们总结了过去几年令人兴奋的观测结果。我们还强调了它们对我们理解FRB种群和提出的祖先模型的影响。我们在之前的评论中介绍了快速射电暴,向读者更新了最近的结果,并讨论了有趣的探索途径,因为该领域进入了一个新的体制,每年都会发现和报道成百上千的新快速射电暴。
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来源期刊
The Astronomy and Astrophysics Review
The Astronomy and Astrophysics Review 地学天文-天文与天体物理
CiteScore
45.00
自引率
0.80%
发文量
7
期刊介绍: The Astronomy and Astrophysics Review is a journal that covers all areas of astronomy and astrophysics. It includes subjects related to other fields such as laboratory or particle physics, cosmic ray physics, studies in the solar system, astrobiology, instrumentation, and computational and statistical methods with specific astronomical applications. The frequency of review articles depends on the level of activity in different areas. The journal focuses on publishing review articles that are scientifically rigorous and easily comprehensible. These articles serve as a valuable resource for scientists, students, researchers, and lecturers who want to explore new or unfamiliar fields. The journal is abstracted and indexed in various databases including the Astrophysics Data System (ADS), BFI List, CNKI, CNPIEC, Current Contents/Physical, Chemical and Earth Sciences, Dimensions, EBSCO Academic Search, EI Compendex, Japanese Science and Technology, and more.
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