A STRONG MERGER SHOCK IN ABELL 665

被引:35
作者
Dasadia, S. [1 ]
Sun, M. [1 ]
Sarazin, C. [2 ]
Morandi, A. [1 ]
Markevitch, M. [3 ]
Wik, D. [3 ,4 ]
Feretti, L. [5 ]
Giovannini, G. [6 ]
Govoni, F. [7 ]
Vacca, V. [7 ]
机构
[1] Univ Alabama, Dept Phys, Huntsville, AL 35816 USA
[2] Univ Virginia, Dept Astron, Charlottesville, VA 22904 USA
[3] NASA, Goddard Space Flight Ctr, Astrophys Sci Div, Greenbelt, MD 20771 USA
[4] Johns Hopkins Univ, Homewood Campus, Baltimore, MD 21218 USA
[5] INAF ORA Bologna, Via Gobetti 101, I-40129 Bologna, Italy
[6] Dipartimento Astron, Via Ranzani 1, I-40127 Bologna, Italy
[7] INAF ORA Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy
基金
美国国家航空航天局;
关键词
galaxies: clusters: general; galaxies: clusters: individual (Abell 665); radio continuum: general; shock waves; X-rays: galaxies: clusters; GALAXY CLUSTERS; X-RAY; RADIO HALOS; BOW SHOCK; INTRACLUSTER MEDIUM; MERGING CLUSTERS; BULLET CLUSTER; COLD FRONTS; CHANDRA; SAMPLE;
D O I
10.3847/2041-8205/820/1/L20
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Deep (103 ks) Chandra observations of Abell 665 have revealed rich structures in this merging galaxy cluster, including a strong shock and two cold fronts. The newly discovered shock has a Mach number of M = 3.0 +/- 0.6, propagating in front of a cold disrupted cloud. This makes Abell 665 the second cluster, after the Bullet cluster, where a strong merger shock of M approximate to 3 has been detected. The shock velocity from jump conditions is consistent with (2.7 +/- 0.7) x 10(3) km s(-1). The new data also reveal a prominent southern cold front with potentially heated gas ahead of it. Abell 665 also hosts a giant radio halo. There is a hint of diffuse radio emission extending to the shock at the north, which needs to be examined with better radio data. This new strong shock provides a great opportunity to study the re-acceleration model with the X-ray and radio data combined.
引用
收藏
页数:5
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