Open Access

Table A.4.

Stellar positions and velocities for Octans members at present time (t = 0) and birth time of the association (t = −34 Myr). This table will be available in its entirety at the CDS.

Source identifier X0 Y0 Z0 U0 V0 W0 X Y Z U V W
(pc) (pc) (pc) (km/s) (km/s) (km/s) (pc) (pc) (pc) (km/s) (km/s) (km/s)
2888316685668937984 49 . 9 0.1 + 0.1 $ -49.9 _{ -0.1 }^{+ 0.1 } $ 87 . 4 0.1 + 0.1 $ -87.4 _{ -0.1 }^{+ 0.1 } $ 56 . 5 0.1 + 0.1 $ -56.5 _{ -0.1 }^{+ 0.1 } $ 4 . 2 0.3 + 0.3 $ -4.2 _{ -0.3 }^{+ 0.3 } $ 9 . 5 0.5 + 0.5 $ 9.5 _{ -0.5 }^{+ 0.5 } $ 3 . 1 0.3 + 0.3 $ -3.1 _{ -0.3 }^{+ 0.3 } $ 28 . 8 12.6 + 11.9 $ 28.8 _{ -12.6 }^{+ 11.9 } $ 366 . 6 17.1 + 16.0 $ -366.6 _{ -17.1 }^{+ 16.0 } $ 72 . 1 2.4 + 2.2 $ 72.1 _{ -2.4 }^{+ 2.2 } $ 1 . 3 0.5 + 0.5 $ 1.3 _{ -0.5 }^{+ 0.5 } $ 7 . 6 0.6 + 0.6 $ 7.6 _{ -0.6 }^{+ 0.6 } $ 0 . 1 0.3 + 0.2 $ 0.1 _{ -0.3 }^{+ 0.2 } $
2889149393928673664 59 . 4 0.1 + 0.1 $ -59.4 _{ -0.1 }^{+ 0.1 } $ 106 . 8 0.2 + 0.2 $ -106.8 _{ -0.2 }^{+ 0.2 } $ 57 . 9 0.1 + 0.1 $ -57.9 _{ -0.1 }^{+ 0.1 } $ 4 . 9 0.3 + 0.3 $ -4.9 _{ -0.3 }^{+ 0.3 } $ 8 . 2 0.5 + 0.5 $ 8.2 _{ -0.5 }^{+ 0.5 } $ 4 . 0 0.3 + 0.3 $ -4.0 _{ -0.3 }^{+ 0.3 } $ 40 . 3 12.6 + 12.4 $ 40.3 _{ -12.6 }^{+ 12.4 } $ 338 . 9 17.8 + 17.3 $ -338.9 _{ -17.8 }^{+ 17.3 } $ 79 . 9 2.0 + 2.0 $ 79.9 _{ -2.0 }^{+ 2.0 } $ 0 . 5 0.5 + 0.5 $ 0.5 _{ -0.5 }^{+ 0.5 } $ 6 . 1 0.6 + 0.6 $ 6.1 _{ -0.6 }^{+ 0.6 } $ 0 . 7 0.2 + 0.2 $ 0.7 _{ -0.2 }^{+ 0.2 } $
2892371925071938944 77 . 1 0.2 + 0.2 $ -77.1 _{ -0.2 }^{+ 0.2 } $ 134 . 2 0.3 + 0.3 $ -134.2 _{ -0.3 }^{+ 0.3 } $ 52 . 9 0.1 + 0.1 $ -52.9 _{ -0.1 }^{+ 0.1 } $ 5 . 7 0.2 + 0.1 $ -5.7 _{ -0.2 }^{+ 0.1 } $ 7 . 7 0.3 + 0.2 $ 7.7 _{ -0.3 }^{+ 0.2 } $ 4 . 2 0.1 + 0.1 $ -4.2 _{ -0.1 }^{+ 0.1 } $ 41 . 3 6.4 + 6.9 $ 41.3 _{ -6.4 }^{+ 6.9 } $ 341 . 6 8.4 + 9.0 $ -341.6 _{ -8.4 }^{+ 9.0 } $ 77 . 9 0.8 + 0.8 $ 77.9 _{ -0.8 }^{+ 0.8 } $ 0 . 2 0.3 + 0.3 $ 0.2 _{ -0.3 }^{+ 0.3 } $ 5 . 4 0.3 + 0.3 $ 5.4 _{ -0.3 }^{+ 0.3 } $ 1 . 1 0.1 + 0.1 $ 1.1 _{ -0.1 }^{+ 0.1 } $
2892719473825487104 67 . 8 0.1 + 0.1 $ -67.8 _{ -0.1 }^{+ 0.1 } $ 119 . 2 0.2 + 0.3 $ -119.2 _{ -0.2 }^{+ 0.3 } $ 54 . 8 0.1 + 0.1 $ -54.8 _{ -0.1 }^{+ 0.1 } $ 5 . 3 0.1 + 0.1 $ -5.3 _{ -0.1 }^{+ 0.1 } $ 8 . 1 0.1 + 0.1 $ 8.1 _{ -0.1 }^{+ 0.1 } $ 4 . 3 0.1 + 0.1 $ -4.3 _{ -0.1 }^{+ 0.1 } $ 42 . 3 3.3 + 3.4 $ 42.3 _{ -3.3 }^{+ 3.4 } $ 343 . 2 4.3 + 4.7 $ -343.2 _{ -4.3 }^{+ 4.7 } $ 80 . 0 0.5 + 0.5 $ 80.0 _{ -0.5 }^{+ 0.5 } $ 0 . 3 0.1 + 0.1 $ 0.3 _{ -0.1 }^{+ 0.1 } $ 5 . 9 0.2 + 0.1 $ 5.9 _{ -0.2 }^{+ 0.1 } $ 1 . 1 0.1 + 0.1 $ 1.1 _{ -0.1 }^{+ 0.1 } $
2893814896644875264 74 . 2 0.1 + 0.1 $ -74.2 _{ -0.1 }^{+ 0.1 } $ 127 . 9 0.2 + 0.2 $ -127.9 _{ -0.2 }^{+ 0.2 } $ 44 . 3 0.1 + 0.1 $ -44.3 _{ -0.1 }^{+ 0.1 } $ 5 . 6 0.1 + 0.1 $ -5.6 _{ -0.1 }^{+ 0.1 } $ 7 . 8 0.2 + 0.2 $ 7.8 _{ -0.2 }^{+ 0.2 } $ 5 . 6 0.1 + 0.1 $ -5.6 _{ -0.1 }^{+ 0.1 } $ 43 . 5 4.4 + 4.8 $ 43.5 _{ -4.4 }^{+ 4.8 } $ 339 . 9 5.9 + 6.4 $ -339.9 _{ -5.9 }^{+ 6.4 } $ 82 . 1 0.5 + 0.5 $ 82.1 _{ -0.5 }^{+ 0.5 } $ 0 . 1 0.2 + 0.2 $ 0.1 _{ -0.2 }^{+ 0.2 } $ 5 . 5 0.2 + 0.2 $ 5.5 _{ -0.2 }^{+ 0.2 } $ 2 . 5 0.1 + 0.1 $ 2.5 _{ -0.1 }^{+ 0.1 } $
2895580295703693056 91 . 2 0.2 + 0.2 $ -91.2 _{ -0.2 }^{+ 0.2 } $ 141 . 4 0.3 + 0.3 $ -141.4 _{ -0.3 }^{+ 0.3 } $ 48 . 7 0.1 + 0.1 $ -48.7 _{ -0.1 }^{+ 0.1 } $ 5 . 2 0.5 + 0.4 $ -5.2 _{ -0.5 }^{+ 0.4 } $ 9 . 0 0.7 + 0.7 $ 9.0 _{ -0.7 }^{+ 0.7 } $ 4 . 4 0.3 + 0.2 $ -4.4 _{ -0.3 }^{+ 0.2 } $ 3 . 7 19.4 + 21.6 $ -3.7 _{ -19.4 }^{+ 21.6 } $ 396 . 4 24.0 + 26.3 $ -396.4 _{ -24.0 }^{+ 26.3 } $ 76 . 2 1.8 + 1.9 $ 76.2 _{ -1.8 }^{+ 1.9 } $ 1 . 6 0.9 + 0.8 $ 1.6 _{ -0.9 }^{+ 0.8 } $ 7 . 2 0.9 + 0.9 $ 7.2 _{ -0.9 }^{+ 0.9 } $ 1 . 3 0.2 + 0.2 $ 1.3 _{ -0.2 }^{+ 0.2 } $
2898428000757810560 86 . 1 0.2 + 0.2 $ -86.1 _{ -0.2 }^{+ 0.2 } $ 127 . 8 0.2 + 0.3 $ -127.8 _{ -0.2 }^{+ 0.3 } $ 53 . 3 0.1 + 0.1 $ -53.3 _{ -0.1 }^{+ 0.1 } $ 6 . 1 0.4 + 0.4 $ -6.1 _{ -0.4 }^{+ 0.4 } $ 7 . 8 0.5 + 0.5 $ 7.8 _{ -0.5 }^{+ 0.5 } $ 4 . 2 0.2 + 0.2 $ -4.2 _{ -0.2 }^{+ 0.2 } $ 44 . 2 15.9 + 16.1 $ 44.2 _{ -15.9 }^{+ 16.1 } $ 342 . 6 18.6 + 19.3 $ -342.6 _{ -18.6 }^{+ 19.3 } $ 78 . 1 1.6 + 1.6 $ 78.1 _{ -1.6 }^{+ 1.6 } $ 0 . 2 0.6 + 0.6 $ -0.2 _{ -0.6 }^{+ 0.6 } $ 5 . 6 0.7 + 0.7 $ 5.6 _{ -0.7 }^{+ 0.7 } $ 1 . 1 0.2 + 0.2 $ 1.1 _{ -0.2 }^{+ 0.2 } $
2917020604947950976 90 . 0 0.3 + 0.3 $ -90.0 _{ -0.3 }^{+ 0.3 } $ 99 . 0 0.3 + 0.3 $ -99.0 _{ -0.3 }^{+ 0.3 } $ 49 . 9 0.2 + 0.1 $ -49.9 _{ -0.2 }^{+ 0.1 } $ 6 . 7 0.2 + 0.3 $ -6.7 _{ -0.2 }^{+ 0.3 } $ 7 . 5 0.3 + 0.3 $ 7.5 _{ -0.3 }^{+ 0.3 } $ 5 . 5 0.1 + 0.1 $ -5.5 _{ -0.1 }^{+ 0.1 } $ 71 . 5 10.7 + 9.8 $ 71.5 _{ -10.7 }^{+ 9.8 } $ 310 . 7 9.9 + 9.3 $ -310.7 _{ -9.9 }^{+ 9.3 } $ 85 . 3 1.0 + 1.0 $ 85.3 _{ -1.0 }^{+ 1.0 } $ 1 . 5 0.4 + 0.4 $ -1.5 _{ -0.4 }^{+ 0.4 } $ 5 . 4 0.3 + 0.4 $ 5.4 _{ -0.3 }^{+ 0.4 } $ 2 . 2 0.1 + 0.1 $ 2.2 _{ -0.1 }^{+ 0.1 } $
4772071921306849792 20 . 0 0.1 + 0.1 $ -20.0 _{ -0.1 }^{+ 0.1 } $ 103 . 4 0.1 + 0.2 $ -103.4 _{ -0.1 }^{+ 0.2 } $ 73 . 3 0.1 + 0.1 $ -73.3 _{ -0.1 }^{+ 0.1 } $ 3 . 5 0.1 + 0.1 $ -3.5 _{ -0.1 }^{+ 0.1 } $ 7 . 4 0.7 + 0.6 $ 7.4 _{ -0.7 }^{+ 0.6 } $ 4 . 3 0.5 + 0.4 $ -4.3 _{ -0.5 }^{+ 0.4 } $ 50 . 5 7.3 + 7.5 $ 50.5 _{ -7.3 }^{+ 7.5 } $ 301 . 7 20.9 + 21.9 $ -301.7 _{ -20.9 }^{+ 21.9 } $ 94 . 8 3.5 + 3.5 $ 94.8 _{ -3.5 }^{+ 3.5 } $ 1 . 0 0.4 + 0.4 $ 1.0 _{ -0.4 }^{+ 0.4 } $ 5 . 0 0.7 + 0.7 $ 5.0 _{ -0.7 }^{+ 0.7 } $ 0 . 3 0.4 + 0.4 $ 0.3 _{ -0.4 }^{+ 0.4 } $
4799008375640297344 32 . 7 0.1 + 0.1 $ -32.7 _{ -0.1 }^{+ 0.1 } $ 103 . 9 0.2 + 0.2 $ -103.9 _{ -0.2 }^{+ 0.2 } $ 71 . 0 0.1 + 0.1 $ -71.0 _{ -0.1 }^{+ 0.1 } $ 3 . 8 0.1 + 0.1 $ -3.8 _{ -0.1 }^{+ 0.1 } $ 8 . 4 0.4 + 0.5 $ 8.4 _{ -0.4 }^{+ 0.5 } $ 3 . 0 0.3 + 0.3 $ -3.0 _{ -0.3 }^{+ 0.3 } $ 39 . 1 7.6 + 7.2 $ 39.1 _{ -7.6 }^{+ 7.2 } $ 339 . 6 15.8 + 14.9 $ -339.6 _{ -15.8 }^{+ 14.9 } $ 83 . 4 2.5 + 2.2 $ 83.4 _{ -2.5 }^{+ 2.2 } $ 1 . 3 0.3 + 0.4 $ 1.3 _{ -0.3 }^{+ 0.4 } $ 6 . 1 0.5 + 0.5 $ 6.1 _{ -0.5 }^{+ 0.5 } $ 0 . 5 0.3 + 0.2 $ -0.5 _{ -0.3 }^{+ 0.2 } $

Notes. We provide for each star the Gaia-DR3 source identifier, 3D positions and 3D velocities at present time (X0, Y0, Z0, U0, V0, W0) and birth time of the association (X, Y, Z, U, V, W) with respect to the LSR. The uncertainties on the stellar positions and velocities were computed from a resampling procedure with 1 000 samples generated from a Gaussian multivariate distribution of the observed parameters (positions, proper motions, parallaxes, and radial velocities) and the full covariance matrix of the data.

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.