Gravitational lenses with more than four images. I. Classification of caustics

被引:26
作者
Keeton, CR [1 ]
Mao, S
Witt, HJ
机构
[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[2] Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[3] Max Planck Inst Astrophys, D-85740 Garching, Germany
[4] Astrophys Inst Potsdam, D-14482 Potsdam, Germany
关键词
distance scale; gravitational lensing;
D O I
10.1086/309087
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the problem of gravitational lensing by an isothermal elliptical density galaxy in the presence of a tidal perturbation. When the perturbation is fairly strong and oriented near the galaxy's minor axis, the lens can produce image configurations with six or even eight highly magnified images lying approximately on a circle. We classify the caustic structures in the model and identify the range of models that can produce such lenses. Sextuple and octuple lenses are likely to be rare because they require special lens configurations, but a full. calculation of the likelihood will have to include both the existence of lenses with multiple-lens galaxies and the strong magnification bias that affects sextuple and octuple lenses. At optical wavelengths, these lenses would probably appear as partial or complete Einstein rings, but at radio wavelengths, the individual images could probably be resolved.
引用
收藏
页码:697 / 707
页数:11
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