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Table 4.

Galactic coordinates, velocities, and main orbital parameters of the stars we studied.

arc tang
Star X Y Z VX VY VZ VR Rmax zmax Lz Vphi Lperp ecc Energy (zmax/
Rmax)
Our sample of turnoff stars with A(Li) compatible with the plateau
BS17572-100 −8.41 −0.33 0.25 8.23 −3.32 19.18 −8.09 8.45 3.84 0.31 3.64 1.64 0.98 −1814 0.43
CS22950-173 −7.63 0.33 −0.37 281.12 17.35 80.71 −280.11 17.16 5.09 −2.25 −29.42 5.12 0.92 −1438 0.29
CS29491-084 −7.67 0.21 −0.94 43.40 48.46 −8.37 −42.06 7.90 1.03 −3.81 −49.63 1.14 0.79 −1833 0.13
CS29514-007 −8.30 0.00 −1.17 −207.90 −361.06 −16.80 208.00 47.10 6.42 29.95 361.00 4.34 0.75 −940 0.14
CS29516-028 −8.02 0.53 −0.50 −86.78 127.08 114.55 95.04 9.35 4.63 −9.72 −121.03 9.70 0.45 −1654 0.46
CS30302-145 −7.18 −0.18 −0.54 72.18 −300.69 −113.72 −64.2 16.86 4.89 21.70 302.45 8.67 0.42 −1354 0.28
CS30344-070 −7.55 0.09 −1.27 −8.43 128.34 −168.80 9.92 8.19 5.90 −9.68 −128.23 12.72 0.19 −1630 0.62
HE1413-1954 −6.97 −0.75 1.16 −175.35 164.93 −7.33 156.63 10.71 2.03 −12.82 −182.81 3.15 0.48 −1604 0.19
HE0148-2611 −8.45 −0.15 −1.17 132.99 −66.46 254.10 −131.82 17.13 16.22 5.81 68.74 19.96 0.51 −1367 0.76
Our sample of turnoff stars with A(Li) significantly lower than the plateau
CS22188-033 −8.16 −0.07 −0.43 −53.61 −9.28 28.02 53.69 8.44 0.74 0.72 8.81 2.52 0.95 −1812 0.09
CS22882-027 −8.10 −0.06 −1.31 −40.62 −160.79 −162.76 41.73 9.95 6.21 13.00 160.51 12.81 0.22 −1549 0.56

Turnoff stars of the First Stars sample with A(Li) significantly lower than the plateau
CS22888-031 −7.85 0.03 −0.85 −215.05 43.68 40.58 215.23 12.54 4.70 −3.36 −4.27 5.02 0.89 −1595 0.36
CS22948-093 −6.87 0.01 −1.62 397.50 97.11 −147.46 −397.42 48.31 42.60 −6.69 −9.74 16.65 0.88 −944 0.72
CS22966-011 −7.96 0.08 −0.84 −42.80 27.84 −14.21 43.07 8.23 3.73 −2.18 −2.74 0.80 0.89 −1823 0.43

Notes. The units are given in the text. We add the parameters of the three Li-poor stars studied in the frame of the First Stars project at the end of the table. The orbital characteristics of the stars studied in the First Stars sample are given in Di Matteo et al. (2020).

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