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Table 4

Kinematic properties of the programme stars.

Name JD RV ΔRV ϵ GRVS source U V W Gaia DR2 Bin./Rem.
(−2 400 000) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1)
No s-process enrichment
HD 7863 57 205 − 27.82 ± 0.34 0.45 0.29 8.09 GDR2 24.95 −23.58 −13.81 397523176280439808 n
58 882.41 − 28.27 ± 0.07 HER
HIP 69788 57 205 6.56 ± 1.94 55.93 0.42 9.39 GDR2 31.08 11.94 −9.27 3667671452515762944 y(a)
58 877.70 − 49.37 ± 0.07 HER
TYC 3144−1906−1 57 205 − 21.56 ± 0.33 1.06 0.28 7.84 GDR2 −20.73 −16.47 −5.61 2077143186195922176 y
59 090.45 − 22.62 ± 0.07 HER
TYC 4684−2242−1 57 205 36.53 ± 0.44 0.92 0.41 9.35 GDR2 −66.36 6.01 −15.01 2478965826587133568 n
58 882.33 35.61 ± 0.07 HER
Mild s-process enrichment
BD − 07° 402 57 205 − 12.96 ± 0.17 0.48 0.29 8.04 GDR2 4.72 −2.66 12.05 2486894817251498240 n
58 882.37 − 13.44 ± 0.07 HER
BD + 44° 575 57 205 − 12.61 ± 0.26 0.50 0.28 7.78 GDR2 28.21 17.09 1.94 340768207120632832 n
58 878.41 − 13.11 ± 0.07 HER
TYC 22−155−1 57 205 − 37.70 ± 0.58 0.35 0.33 8.71 GDR2 −48.38 −65.05 32.26 2539172197106047872 n
58 882.36 − 38.05 ± 0.07 HER
TYC 2913−1375−1 57205 − 2.89 ± 0.42 0.15 0.48 9.70 GDR2 2.22 −14.52 44.81 193703372946249216 n
59 090.71 − 3.04 ± 0.07 HER
TYC 3305−571−1 57 205 − 57.93 ± 0.33 0.52 0.37 9.08 GDR2 30.31 −55.92 3.80 437946515118550016 n
58 878.48 − 58.45 ± 0.07 HER
TYC 4837−925−1 57 205 − 22.91 ± 0.23 0.52 0.37 9.11 GDR2 35.55 −8.52 −13.98 3081162263449705984 n
58 877.55 − 23.43 ± 0.07 HER
TYC 3423−696−1 57 205 5.37 ± 0.21 − 3.16 0.40 9.26 GDR2 −21.20 −55.96 −2.78 1016739606459940608 y
58 877.61 8.53 ± 0.07 HER
TYC 752−1944−1 58 877.49 19.04 ± 0.07 HER 4.66 −17.38 −29.26 3157928756551254400 ?
Strong s-process enrichment
TYC 2250−1047−1 57 205 19.39 ± 0.75 3.44 0.75 10.41 GDR2 −76.78 4.84 −9.30 2839977000550809856 y
59 090.61 15.95 ± 0.07 HER
TYC 2955−408−1 57 205 41.15 ± 0.56 2.07 0.42 9.41 GDR2 −61.94 −6.77 −42.54 953203601197511808 y
58 879.54 39.08 ± 0.07 HER
TYC 591−1090−1 57205 8.80 ± 0.88 1.55 1.00 10.83 GDR2 41.23 26.56 9.10 2757528128276067840 n
59 090.64 7.25 ± 0.07 HER

Notes. In column ‘source’, GDR2 stands for Gaia Data Release 2, and ‘HER’ for HERMES. ΔRV is the difference between the HERMES and GDR2 radial velocities. ϵ is the uncertainty on the GDR2 RV, computed as explained in the text. GRVS is the magnitude in the RVS band (Jordi 2018). U, V, W are the Cartesian components of the velocity in Galactic coordinates, taken from N19. The Gaia DR2 identifier has been listed to ease the cross match with N19 data table. For the criteria used to classify stars as ‘no s-process’, ‘mild s-process enrichment’ and ‘strong s-process enrichment’, see Sect. 5. (a)Also proper motion anomaly (Kervella et al. 2019).

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