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Table 7

Radial velocities and Galactic spatial-velocity components for the observed stars.

HIP/ V r* U LSR V LSR W LSR C
Other (km s-1) (km s-1) (km s-1) (km s-1)
(1) (2) (3) (4) (5) (6)

Giants with planets

1692 17.58 ± 0.25 –8.80 ± 8.15 3.94 ± 3.75 –10.75 ± 0.94 D
4297 –0.21 ± 0.31 25.28 ± 1.68 –13.56 ± 2.00 –5.40 ± 1.33 D
10085 25.36 ± 0.46 –13.81 ± 3.55 22.85 ± 3.10 8.97 ± 6.33 D
12247 8.60 ± 0.31 3.65 ± 0.49 –20.57 ± 1.33 –0.63 ± 0.41 D
HD17092 5.56 ± 0.31 –7.50 ± 6.73 –7.26 ± 8.17 8.42 ± 1.49 D

Notes.Only the first five lines are shown here; the full version of the table is available at the CDS. The assumed solar motion with respect to the LSR is (U, V, W) = (10.0, 5.25, 7.17) km s-1 (Dehnen & Binney 1998).

(*)

For those stars in binary systems, we have considered the radial velocity of the centre of mass of the system.

(†)

Thin/thick disk classification, D: thin disk, TD: thick disk, R: transition.

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