Table A.2
Summary of the positional and kinematic properties for all clusters within the CrA, LCC, and Upper−Sco cluster chains.
cluster chains | number of stars | X | Y | Z | dist. | U | V | W | age | |||
---|---|---|---|---|---|---|---|---|---|---|---|---|
total | RVs | final | heliocentric Gal. | Cartesian coord. | [pc] | [pc] | heliocentric Gal. | Cartesian vel. | [km/s] | [Myr] | ||
CrA | ϕ Lup | 1114 | 455 | 53* | 112.4 ± 9.2 | −54.2 ± 6.8 | 40.3 ± 5.9 | 131 | −5.5 ± 1.3 | −19.6 ± 0.7 | −5.5 ± 1.0 | 16.9 |
η Lup | 769 | 360 | 45* | 124.6 ± 7.0 | −46.7 ± 8.8 | 24.7 ± 6.0 | 136 | −4.7 ± 0.9 | −20.0 ± 1.0 | −5.2 ± 0.5 | 15.3 | |
V1062−Sco | 1029 | 309 | 21* | 167.9 ± 4.5 | −51.3 ± 5.8 | 14.4 ± 2.7 | 177 | −3.6 ± 1.0 | −19.6 ± 0.4 | −4.2 ± 0.2 | 15.0 | |
Sco-Sting | 132 | 42 | 7 | 131.3 ± 7.2 | −22.3 ± 5.3 | −7.5 ± 8.1 | 134 | −7.0 ± 1.5 | −18.6 ± 1.0 | −5.3 ± 0.3 | 14.5 | |
CrA-North | 351 | 134 | 11* | 144.7 ± 3.8 | −2.5 ± 2.7 | −36.2 ± 4.3 | 149 | −5.6 ± 0.8 | −17.3 ± 0.5 | −7.8 ± 0.7 | 11.6 | |
CrA-Main | 96 | 56 | 29* | 147.5 ± 2.2 | −0.3 ± 0.7 | −46.9 ± 1.1 | 155 | −4.3 ± 0.6 | −17.5 ± 0.6 | −9.6 ± 0.6 | 8.5 | |
LCC | σ Cen | 1805 | 822 | 99* | 59.9 ± 8.0 | −96.1 ± 7.1 | 17.1 ± 7.6 | 115 | −8.5 ± 1.0 | −20.7 ± 1.1 | −6.2 ± 0.8 | 15.5 |
Acrux | 394 | 190 | 24* | 53.6 ± 2.3 | −91.5 ± 3.5 | −3.6 ± 3.4 | 106 | −9.3 ± 0.6 | −20.0 ± 0.8 | −7.7 ± 0.2 | 11.2 | |
Musca-fg | 95 | 44 | 8 | 51.8 ± 2.1 | −86.5 ± 2.6 | −18.2 ± 2.6 | 102 | −10.2 ± 0.7 | −18.7 ± 1.8 | −8.7 ± 0.4 | 10.2 | |
η Cham | 30 | 14 | 4 | 34.9 ± 0.4 | −84.7 ± 1.0 | −36.2 ± 1.8 | 99 | −11.7 ± 0.7 | −19.3 ± 0.2 | −10.6 ± 0.4 | 9.4 | |
ϵ Cham | 39 | 20 | 4 | 49.8 ± 1.0 | −84.6 ± 1.7 | −27.9 ± 1.0 | 102 | −10.2 ± 0.7 | −19.7 ± 0.7 | −10.5 ± 1.1 | 8.8 | |
Upper−Sco | ϕ Lup | 1114 | 455 | 53* | 112.4 ± 9.2 | −54.2 ± 6.8 | 40.3 ± 5.9 | 131 | −5.5 ± 1.3 | −19.6 ± 0.7 | −5.3 ± 1.0 | 16.9 |
η Lup | 769 | 360 | 45* | 124.6 ± 9.8 | −46.7 ± 8.8 | 24.7 ± 6.0 | 136 | −4.7 ± 0.9 | −20.0 ± 1.0 | −5.2 ± 0.5 | 15.3 | |
Sco-Body | 373 | 143 | 17* | 137.7 ± 7.0 | −26.1 ± 5.6 | 17.3 ± 10.5 | 141 | −3.9 ± 1.4 | −16.8 ± 0.6 | −7.6 ± 0.5 | 14.7 | |
ρ Sco | 240 | 108 | 48* | 129.2 ± 5.2 | −24.5 ± 7.2 | 42.9 ± 3.7 | 139 | −4.3 ± 1.1 | −18.1 ± 0.4 | −4.0 ± 0.5 | 13.7 | |
Antares | 502 | 270 | 131* | 131.7 ± 5.9 | −16.6 ± 4.0 | 41.3 ± 3.8 | 139 | −3.9 ± 1.1 | −16.0 ± 0.7 | −5.8 ± 0.5 | 12.7 | |
σ Sco | 544 | 263 | 158* | 149.3 ± 4.9 | −23.6 ± 3.1 | 49.0 ± 3.2 | 159 | −4.2 ± 1.0 | −17.2 ± 0.7 | −6.2 ± 0.5 | 10.0 | |
δ Sco | 691 | 451 | 268* | 129.7 ± 2.8 | −22.5 ± 4.3 | 53.7 ± 3.0 | 142 | −6.2 ± 0.7 | −16.2 ± 0.5 | −7.6 ± 0.6 | 9.8 | |
β Sco | 285 | 186 | 107* | 140.8 ± 3.8 | −16.6 ± 2.5 | 61.0 ± 3.2 | 154 | −3.0 ± 0.8 | −16.2 ± 0.4 | −6.8 ± 0.6 | 7.6 | |
ν Sco | 150 | 102 | 70* | 127.9 ± 2.4 | −12.3 ± 1.3 | 54.2 ± 1.3 | 139 | −5.2 ± 0.6 | −15.4 ± 0.4 | −9.0 ± 0.4 | 5.8 | |
ρ Oph | 535 | 281 | 155* | 131.6 ± 2.8 | −15.8 ± 1.0 | 40.9 ± 1.9 | 139 | −5.7 ± 0.9 | −15.2 ± 0.6 | −9.2 ± 0.8 | 3.8 |
Notes. Columns 3-5 list the number of stars per cluster, the number of radial velocities, and the final number of radial velocities after applying the selection criteria, including the radial velocity uncertainty cut at 1 km s−1 and sigma-clipping of the radial velocity distribution. Clusters that underwent sigma-clipping are marked with an asterisk (*). See Sect. 2 for details. Columns 6-8 list the median and median absolute deviation (MAD) of each cluster’s position in heliocentric Galactic Cartesian coordinates. The distance to each cluster is given in column 8 and is sourced directly from R23a. Columns 10-12 list the median and MAD of each velocity component in heliocentric Galactic Cartesian coordinates. The cluster ages estimated by R23b are given in column 13.
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.