The Large Magellanic Cloud as a source of the highest energy cosmic rays

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Roger Clay , Tadeusz Wibig
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引用次数: 0

Abstract

The Pierre Auger Observatory has published properties of the 100 highest-energy cosmic ray events (to energies above 100 EeV) which it recorded over a 17 year period. We have examined the directional properties of these events and have taken particular note of the most energetically extreme events. We find that the most energetic events have directions which are grouped in a non-random way at the 1 % level. There is an apparent clustering in a limited region of the sky. Close to that direction is found Centaurus A, which has long been considered as a source of such particles, but we also note that a close-by dwarf galaxy, the Large Magellanic Cloud (LMC) is closer in angular terms. We examine the possibility that the LMC might be a source of observed cosmic rays at the highest energies.
大麦哲伦星云是最高能量宇宙射线的来源
皮埃尔·奥格天文台公布了它在17年期间记录的100个最高能量宇宙射线事件(能量超过100 EeV)的特性。我们已经研究了这些事件的方向性,并特别注意到了能量最极端的事件。我们发现,在1%的水平上,最有能量的事件具有以非随机方式分组的方向。在天空的一个有限区域有一个明显的星团。在这个方向附近发现了半人马座A,它一直被认为是这种粒子的来源,但我们也注意到附近的一个矮星系,大麦哲伦星云(LMC)在角度上更近。我们研究了LMC可能是观测到的最高能量宇宙射线的来源的可能性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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