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Table 2

Dynamical properties of rich clusters.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

Scl ID No ID N comp v pec v rpec p SW k p k sk p sk
SCl 91 1 1066 1 –312 0.41 0.074 2.34 0.139 –0.243 0.528
2 1205 5 49 0.08 0.247 2.37 0.099 –0.069 0.841
SCl 111 3 1424 2 –825 1.26 0.173 2.51 0.387 0.383 0.339
4 1516 1 –58 0.07 0.535 2.84 0.948 –0.292 0.403
SCl 126 5 1650 ×  1 –189 0.41 0.110 2.80 0.946 0.563 0.263
6 1658 ×  1 –463 1.05 0.937 2.37 0.583 0.048 0.936
7 1663 ×  2 –841 1.59 0.372 2.57 0.493 –0.228 0.562
8 1750 ×  5 –724 1.10 0.115 2.51 0.243 –0.265 0.422
9 1773 ×  1 –76 0.12 0.572 3.24 0.436 –0.083 0.835
10 1809 2 –115 0.18 0.802 2.73 0.780 0.053 0.887

Notes. Columns in the table are as follows: 1–3: supercluster ID, cluster No and Abell ID, Col. 4: number of components, Col. 5: peculiar velocity of the first ranked galaxy (km s-1), Col. 6: normalised peculiar velocity of the first ranked galaxy, vpec/σv; Col. 7: p-value of the Shapiro-Wilk test, Cols. 8 and 9: kurtosis k and the p-value pk for kurtosis for the peculiar velocities, Cols. 10 and 11: skewness sk and the p-value psk for skewness for the peculiar velocities.

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