A MEASUREMENT OF THE SUNYAEV-ZELDOVICH EFFECT IN THE COMA CLUSTER OF GALAXIES

被引:92
作者
HERBIG, T [1 ]
LAWRENCE, CR [1 ]
READHEAD, ACS [1 ]
GULKIS, S [1 ]
机构
[1] CALTECH,JET PROP LAB,PASADENA,CA 91125
关键词
COSMIC MICROWAVE BACKGROUND; DISTANCE SCALE; GALAXIES; CLUSTERS; INDIVIDUAL; (COMA);
D O I
10.1086/309616
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the detection of the Sunyaev-Zel'dovich effect in the Coma cluster of galaxies with the 5.5 m telescope at the Owens Valley Radio Observatory. The measured decrement of the temperature of the cosmic microwave background is Delta T-0,T-obs,obs -270 +/- 29 mu K After correcting for the effect of discrete radio sources and applying current models for the X-ray atmosphere of the cluster, we calculate the peak of the effect to be Delta T-0(0) = -505 +/- 92 mu K. Using the same X-ray models, and assuming spherical symmetry for the gas atmosphere, we derive a Hubble constant of H-0= 71(-25)(+30) km s(-1) Mpc(-1). This is the first detection of the Sunyaev-Zel'dovich effect in a nearby cluster of galaxies.
引用
收藏
页码:L5 / L8
页数:4
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