2000ApJ...537..697K


Query : 2000ApJ...537..697K

2000ApJ...537..697K - Astrophys. J., 537, 697-707 (2000/July-2)

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

KEETON C.R., MAO S. and WITT H.J.

Abstract (from CDS):

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.

Abstract Copyright: ∼

Journal keyword(s): Cosmology: Distance Scale - Cosmology: Gravitational Lensing

Simbad objects: 12

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Number of rows : 12
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 8C 0958+561 QSO 10 01 20.6918953728 +55 53 55.593949272   17.16 16.95     ~ 757 3
2 QSO B1115+080A QSO 11 18 16.951 +07 45 58.23   16.61 16.44     ~ 703 2
3 NVSS J113000+381203 Rad 11 30 00.110 +38 12 03.23           ~ 31 0
4 4C 05.51 rG 11 31 56.493 +04 55 48.85           ~ 123 1
5 QSO B1359+154 QSO 14 01 35.588 +15 13 24.15     21.90     ~ 73 1
6 QSO B1422+2309 BLL 14 24 38.0938 +22 56 00.587   16.77 15.84 14.79   ~ 464 1
7 [PBW92] 1422+231 gLS 14 24 38.09400 +22 56 00.5900   16.77 15.84 14.79   ~ 359 0
8 NVSS J160914+653229 rG 16 09 13.93704 +65 32 27.9024     19.4     ~ 215 0
9 CLASS B1933+503 Rad 19 34 31.02 +50 25 23.5           ~ 85 1
10 QSO B2016+112B QSO 20 19 18.0 +11 27 13     22.5     ~ 32 0
11 QSO B2016+112 QSO 20 19 18.2 +11 27 14     22.5     ~ 195 1
12 PKS 2114+022 Rad 21 16 50.74522099 +02 25 46.2623664           ~ 59 1

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