A lensed arc in the low-redshift cluster Abell 2124

被引:11
作者
Blakeslee, JP [1 ]
Metzger, MR [1 ]
机构
[1] CALTECH, Palomar Observ, Pasadena, CA 91125 USA
关键词
galaxies : clusters : individual (Abell 2124); gravitational lensing; galaxies : elliptical and lenticular; cD;
D O I
10.1086/306906
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of an arclike object 27 " from the center of the cD galaxy in the redshift z = 0.066 cluster A2124. Observations with the Keck II telescope reveal that the object is a background galaxy at z = 0.573, apparently lensed into an are of length similar to 8." 5 and total R magnitude m(R) = 20.86 +/- 0.07. The width of the are is resolved; we estimate it to be similar to 0." 6 after correcting for seeing. A lens model of the A2124 core mass distribution consistent with the cluster galaxy velocity dispersion reproduces the observed are geometry and indicates a magnification factor greater than or similar to 9. With this magnification, the strength of the [O II] lambda 3727 line implies a star formation rate of similar to 0.4 h(-2) M-circle dot yr(-1). A2124 thus appears to be the lowest redshift cluster known to exhibit strong lensing of a distant background galaxy.
引用
收藏
页码:592 / 597
页数:6
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