2001ApJ...557..594R


Query : 2001ApJ...557..594R

2001ApJ...557..594R - Astrophys. J., 557, 594-604 (2001/August-3)

B1359+154: a six-image lens produced by a z ≃ 1 compact group of galaxies.

RUSIN D., KOCHANEK C.S., NORBURY M., FALCO E.E., IMPEY C.D., LEHAR J., McLEOD B.A., RIX H.-W., KEETON C.R., MUNOZ J.A. and PENG C.Y.

Abstract (from CDS):

Hubble Space Telescope (HST) V- and I-band observations show that the gravitational lens B1359+154 consists of six images of a single zs=3.235 radio source and its star-forming host galaxy, produced by a compact group of galaxies at zl≃1. Very Long Baseline Array (VLBA) observations at 1.7 GHz strongly support this conclusion, showing six compact cores with similar low-frequency radio spectra. B1359+154 is the first example of galaxy-scale gravitational lensing in which more than four images are observed of the same background source. The configuration is due to the unique lensing mass distribution: three primary lens galaxies lying on the vertices of a triangle separated by 0".7≃4 h–1 kpc, inside the 1".7 diameter Einstein ring defined by the radio images. The gravitational potential has additional extrema within this triangle, creating a pair of central images that supplement the ``standard'' four-image geometry of the outer components. Simple mass models, consisting of three lens galaxies constrained by HST and VLBA astrometry, naturally reproduce the observed image positions but must be finely tuned to fit the flux densities.

Abstract Copyright:

Journal keyword(s): Galaxies: Clusters: General - Cosmology: Gravitational Lensing

Nomenclature: Table 2, Fig.4: [RKN2001] G, <%M [RKN2001] G'>, [RKN2001] G'' N=3. Table 3: [RKN2001] ANN (Nos G1-G11, S1-S2, T1-T3).

Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 23

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Number of rows : 23
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 ZwCl 0024+1652 ClG 00 26 35.6 +17 09 32     18.35     ~ 636 1
2 4C 05.19 QSO 04 14 37.76734974 +05 34 42.3295956   24.100 23.800 21.270   ~ 360 2
3 [VV2006] J083105.4+522520 QSO 08 31 05.4 +52 25 21     19.60     ~ 14 3
4 QSO J0831+5245 QSO 08 31 41.7108197808 +52 45 17.616994560   19.2   14.5 13.9 ~ 555 1
5 [VV2006] J092112.8+452905 QSO 09 21 12.8304560016 +45 29 03.987252096   19.09 18.71     ~ 37 2
6 8C 0958+561 QSO 10 01 20.6918953728 +55 53 55.593949272   17.16 16.95     ~ 737 3
7 QSO B1030+074 QSO 10 33 34.02429368 +07 11 26.1475933     20.34 20.22   ~ 107 2
8 QSO B1115+080A QSO 11 18 16.951 +07 45 58.23   16.61 16.44     ~ 686 2
9 NVSS J113000+381203 Rad 11 30 00.110 +38 12 03.23           ~ 31 0
10 4C 05.51 G 11 31 56.5 +04 55 49           ~ 123 1
11 [VV2000] J115518.3+193942 QSO 11 55 18.2955044232 +19 39 42.228456840   17.15 16.89     ~ 97 2
12 [RNB2002] G G 11 55 18.33 +19 39 41.4           ~ 23 1
13 [MRF99] CLASS B1359+154 B LeI 14 01 35.5157 +15 13 24.387           ~ 4 0
14 [MRF99] CLASS B1359+154 C LeI 14 01 35.5281 +15 13 23.981           ~ 4 0
15 [MRF99] CLASS B1359+154 A LeI 14 01 35.5495 +15 13 25.643           ~ 4 0
16 [MRF99] CLASS B1359+154 F LeI 14 01 35.5797 +15 13 24.688           ~ 4 0
17 QSO B1359+154 QSO 14 01 35.588 +15 13 24.15     21.90     ~ 73 1
18 [MRF99] CLASS B1359+154 E LeI 14 01 35.5921 +15 13 24.505           ~ 4 0
19 [MRF99] CLASS B1359+154 D LeI 14 01 35.6157 +15 13 24.271           ~ 4 0
20 NVSS J160914+653229 rG 16 09 13.96 +65 32 28.8     19.4     ~ 207 0
21 QSO B2016+112 QSO 20 19 18.2 +11 27 14     22.5     ~ 194 1
22 [VV2000] J204719.3+264340 QSO 20 47 20.3 +26 44 03     20.60     ~ 110 2
23 FIRST J232140.7+052737 Rad 23 21 40.801 +05 27 37.23           ~ 28 1

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