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Table 4.

Distance and spatial velocity of the Lupus subgroups in our sample of cluster members.

Sample Nd NUVW d U V W
(pc) (km s−1)
(km s−1)
(km s−1)
Mean ± SEM Median SD Mean ± SEM Median SD Mean ± SEM Median SD
Lupus 1 4 2 −5.5 ± 1.8 −5.5 2.5 −17.5 ± 1.2 −17.5 1.7 −6.9 ± 0.2 −6.9 0.3
Lupus 2 2 2 −5.8 ± 0.5 −5.8 0.7 −17.4 ± 0.1 −17.4 0.1 −7.3 ± 0.1 −7.3 0.2
Lupus 3 56 35 −3.5 ± 0.5 −3.6 3.1 −17.6 ± 0.3 −17.5 1.5 −7.5 ± 0.2 −7.5 0.9
Lupus 4 18 7 −4.3 ± 0.6 −4.3 1.7 −17.9 ± 0.4 −18.2 1.0 −7.3 ± 0.2 −7.1 0.5
Lupus 5 2 0
Lupus 6 1 0
Lupus (off-cloud) 30 4 −3.7 ± 2.0 −4.4 3.9 −17.2 ± 0.8 −17.4 1.6 −7.1 ± 0.4 −7.3 0.9

Lupus (all stars) 113 50 −3.8 ± 0.4 −4.4 2.9 −17.6 ± 0.2 −17.5 1.4 −7.4 ± 0.1 −7.4 0.8

Notes. We provide for each subgroup the number of stars used to compute the distance (after the RUWE filtering) and spatial velocity, Bayesian distance, mean, standard error of the mean (SEM), median, and standard deviation (SD) of the UVW velocity components.

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