Table 3
Structures detected along the line of sight to the two candidate clusters.
| Name | # | N gal | z | Vel. disp. (km s-1) | SG substructures |
|
|
|||||
| D3-6 | 1 | 8 | 0.607 | 423 | 1 |
|
|
|||||
| D3-43 | S1 | 17 | 0.201 | 489 | / |
| S2 | 11 | 0.378 | 250 | / | |
| S3 | 46 | 0.739 | 1152 | 2 | |
| S4 | 18 | 0.975 | 575 | / | |
Notes. The columns are: (1) cluster name; (2) number of the structure; (3) number of galaxies in the structure; (4) mean redshift of the structure; (5) Rostat velocity dispersion; (6) number of substructures when analysed by the Serna & Gerbal (1996) method.
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