Table 2.
Properties of the different cluster substructures (see Fig. 3).
| Substructure | RA (J2000) | Dec | Radius (a) | Velocity range (b) | Dist (c) | ⟨vel⟩ | σ | Central galaxy |
|---|---|---|---|---|---|---|---|---|
| (°) | (°) | (°) | (km s−1) | (Mpc) | (km s−1) | (km s−1) | ||
| Cluster A | 187.71 | 12.39 | < 5.383 | < 3000 | 16.5 | 955 | 799 | M 87 |
| Cluster B | 187.44 | 8.00 | < 3.334 | < 3000 | 23 | 1134 | 464 | M 49 |
| Cluster C | 190.85 | 11.45 | < 0.7 | < 3000 | 16.5 | 1073 | 545 | M 60 |
| W cloud | 185.00 | 5.80 | < 1.2 | 1000 < vhel < 3000 | 32 | 2176 | 416 | NGC 4261 |
| W′ cloud | 186.00 | 7.20 | < 0.8 | < 2000 | 23 | 1019 | 416 | NGC 4365 |
| M cloud | 183.00 | 13.40 | < 1.5 | 1500 < vhel < 3000 | 32 | 2109 | 280 | NGC 4168 |
| LVC cloud | 184.00 | 13.40 | < 1.5 | vhel < 400 | 16.5 | 85 | 208 | NGC 4216 |
Notes. Galaxies in the overlapping regions that satisfy the membership criteria of two different structures are assumed to be members of the smallest structure for clusters C, W, W′, M, and the LVC clouds. Those in the overlapping region between clusters A and B are assigned to the substructure whose centre is closest to the galaxy.
Radius used to identify the different substructures. For clusters A and B, this corresponds to the r200 radius from Ferrarese et al. (2012).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.