连接两个星系团的无线电脊
F Govoni1, E Orrù2, A Bonafede3,4,5
1Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Cagliari Via della Scienza 5, I09047 Selargius, Italy. federica.govoni@inaf.it.
概括
在合并的星系团Abel 0399和Abel 0401之间检测到的无线电辐射表明有磁场和重新加速的粒子. 这种由LOFAR望远镜观察到的现象可能是由微弱的冲击引起的.
科学领域:
- 宇宙学
- 天体物理学
- 无线电天文学
背景情况:
- 星系团是最大的引力结合的结构.
- 星系团的合并会在星系团内的气体中产生冲击和流.
- 相对论粒子和磁场是宇宙结构的关键组成部分.
研究的目的:
- 为了研究连接星系团Abel 0399和Abel 0401的无线电辐射山脊.
- 了解相对论电子和磁场在集群间丝线中的起源.
- 在星系团外围的粒子加速中探索冲击的作用.
主要方法:
- 使用低频阵列 (LOFAR) 望远镜对140 MHz的无线电发射进行观测.
- 分析连接两个星系团的无线电发射脊.
- 宇宙模拟模型粒子加速机制.
主要成果:
- 在Abel 0399和Abel 0401之间检测到无线电辐射.
- 辐射表明相对论电子和磁场存在于集群间的光线中.
- 模拟表明微弱的冲击可以重新加速已经存在的相对论粒子.
结论:
- 观察到的无线电发射可能是由磁丝中的相对论粒子重新加速引起的.
- 在整个体积中分布的微弱冲击可能负责激发这些粒子.
- 这一发现揭示了宇宙网络中的粒子加速过程.
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