Details on Acronym: [FLH92] | |
| [FLH92] | (Fort+Le Fevre+Hammer+, 1992) |
| Write: | <<[FLH92] GNN>> <<[FLH92] GNN'>> <<[FLH92] ANN>> <<[FLH92] ANN SKN>> <<[FLH92] AR>> <<[FLH92] ARN>> |
| N: | 32+1+11+3+4 |
| Object: | G + Arc (SIMBAD class: Galaxy) |
| Stat: | is completely incorporated in Simbad |
| Note: | (Nos G1-G32) Galaxies in the lensing cluster MS 2137-23 = 1E 2137.3-2353 (Nos A0-A10) for Arcs (sources of these arcs are [HGS97] S1 to S3 sources). Giant tangential arc A0 is broken in 3 segments A01, A02, A03. AO1 and A02 are subdivided in 2 'subknots' SK1 and SK2. 'AR' and 'ARN' are 2 radial arcs (ARN North of AR). |
| in source: | 1E 2137.0-2353 |
| Ref: | =1992ApJ...399L.125F |
| by | FORT B. , LE FEVRE O., HAMMER F., CAILLOUX M. |
| Astrophys. J., 399, 125-127 (1992) | |
| An arc system with a radial gravitational image in the cluster MS 2137-23. | |
| o | Table 1: Table 1: <[FLH92] GNN> (Nos G1-G32), <[FLH92] ANN> (Nos A0, A01, A02, A1-A10) |
| Ref: | =1993ApJ...407...33M |
| by | MELLIER Y. , FORT B., KNEIB J.-P. |
| Astrophys. J., 407, 33-45 (1993) | |
| The dark matter distribution in MS 2137-23 from the modeling of the multiple arc systems. | |
| o | MS 2137-23 = 1E 2137.3-2353, Radial Arc later designated as [FLH92] AR. |
| o | Fig.4: <[FLH92] A03> N=1 added, <[FLH92] GNN'> (No. G29') added. |
| Ref: | =1997ApJ...491..477H |
| by | HAMMER F. , GIOIA I.M., SHAYA E.J., TEYSSANDIER P., LE FEVRE O., LUPPINO G.A. |
| Astrophys. J., 491, 477-482 (1997) | |
| Detailed lensing properties of the MS 2137-2353 core and reconstruction of sources from Hubble Space Telescope imagery. | |
| o | Fig.2: <[FLH92] AR> N=1 added, <[FLH92] ARN> N=1 added, <[FLH92] A01 SKN> (Nos SK1-SK2) added, <[FLH92] A02 SKN> (Nos SK1-SK2) added. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |