A M ≳ 3 shock in 'El Gordo' cluster and the origin of the radio relic

被引:66
作者
Botteon, A. [1 ,2 ]
Gastaldello, F. [3 ]
Brunetti, G. [2 ]
Kale, R. [4 ]
机构
[1] Univ Bologna, Dipartimento Fis & Astron, Via C Ranzani 1, I-40127 Bologna, Italy
[2] INAF IRA, Via P Gobetti 101, I-40129 Bologna, Italy
[3] INAF IASF Milano, Via E Bassini 15, I-20133 Milan, Italy
[4] Tata Inst Fundamental Res, Natl Ctr Radio Astrophys, Pune 411007, Maharashtra, India
关键词
radiation mechanisms: non-thermal; shock waves; galaxies: clusters: individual: ACT-CL J0102-4915; radio continuum: general; X-rays: galaxies: clusters; NONTHERMAL ELECTRON ACCELERATION; X-RAY EXCESS; COMA CLUSTER; MERGING CLUSTER; PARTICLE-ACCELERATION; GALAXY CLUSTERS; EMISSION; FRONTS; EFFICIENCY; RADIATION;
D O I
10.1093/mnras/stw2089
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an X-ray and radio study of the famous 'El Gordo', a massive and distant (z = 0.87) galaxy cluster. In the deep (340 ks) Chandra observation, the cluster appears with an elongated and cometary morphology, a sign of its current merging state. The GMRT radio observations at 610 MHz confirm the presence of a radio halo, which remarkably overlaps the X-ray cluster emission and connects a couple of radio relics. We detect a strong shock (M greater than or similar to 3) in the NW periphery of the cluster, co-spatially located with the radio relic. This is the most distant (z = 0.87) and one of the strongest shocks detected in a galaxy cluster. This work supports the relic shock connection and allows us to investigate the origin of these radio sources in an uncommon regime of M greater than or similar to 3. For this particular case we found that shock acceleration from the thermal pool is still a viable possibility.
引用
收藏
页码:1534 / 1542
页数:9
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