Giant ringlike radio structures around galaxy cluster Abell 3376

被引:153
|
作者
Bagchi, Joydeep
Durret, Florence
Lima Neto, Gastao B.
Paul, Surajit
机构
[1] IUCAA, Pune 411007, Maharashtra, India
[2] Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, Paris, France
[3] Observ Paris, LERMA, Paris, France
[4] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfericas, BR-05508900 Sao Paulo, Brazil
[5] Univ Wurzburg, Inst Theoret Phys & Astrophys, D-97070 Wurzburg, Germany
关键词
D O I
10.1126/science.1131189
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
In the current paradigm of cold dark matter cosmology, large-scale structures are assembling through hierarchical clustering of matter. In this process, an important role is played by megaparsec (Mpc) - scale cosmic shock waves, arising in gravity-driven supersonic flows of intergalactic matter onto dark matter - dominated collapsing structures such as pancakes, filaments, and clusters of galaxies. Here, we report Very Large Array telescope observations of giant (similar to 2 Mpc by 1.6 Mpc), ring-shaped nonthermal radio-emitting structures, found at the outskirts of the rich cluster of galaxies Abell 3376. These structures may trace the elusive shock waves of cosmological large-scale matter flows, which are energetic enough to power them. These radio sources may also be the acceleration sites where magnetic shocks are possibly boosting cosmic-ray particles with energies of up to 10(18) to 10(19) electron volts.
引用
收藏
页码:791 / 794
页数:4
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