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Table 2

Properties of the two clusters.

Cluster αICRS (deg) δICRS (deg) Age (Ga) Distance (kpc) X (kpc) Y (kpc) Z (kpc) RGC (kpc) AV (mag)
Auner 1 106.06 −19.748 3.2 ± 0.7 7.460.57+0.66$^{+0.66}_{-0.57}$ −12.7 ± 0.4 −5.9 ± 0.5 −0.78 ± 0.06 14.1 ±0.5 1.35 ± 0.03
Berkeley 102 354.66 56.637 3.2 ± 0.7 8.260.91+1.16$8.26^{+1.16}_{-0.91}$ −11.40 ± 0.05 7.7 ± 1.1 −0.68 ± 0.10 13.8 ± 1.0 1.32 ± 0.12
NRV vrad,OC σvrad,OC evrad,OC vGSR vRSR Us Vs Ws Vφ
(km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1)
Auner 1 4 37.17 0.66 0.33 −68.0 ± 0.7 25.3 ± 2.7 −25.5 ± 2.8 −38.5 ± 2.8 0.8 ± 5.9 182.9 ± 2.9
Berkeley 102 3 −86.85 3.45 1.99 139.6 ± 3.6 30.3 ± 4.2 −22.8 ± 4.1 −4.2 ± 3.1 20.4 ± 4.1 217.1 ± 3.4
NABU [Fe/H] [Ca/Fe] [Ti/Fe] [Co/Fe] [Ni/Fe] [Ba/Fe] [Eu/Fe]
(dex) (dex) (dex) (dex) (dex) (dex) (dex)
Auner 1 3 −0.30 ± 0.10 0.17 ± 0.18 0.20 ± 0.26a 0.05 ±0.17a 0.05 ± 0.08 0.22 ± 0.10
Berkeley 102 3 −0.35 ± 0.07 0.19 ± 0.15 0.12 ± 0.09 −0.02 ± 0.10 0.01 ± 0.05 0.33 ± 0.14 0.64 ± 0.05 a

Notes. First rows: Main cluster parameters derived from Gaia DR3 (see Sect. 3.1 for details). Middle rows: kinematics (Sects. 3.3 through 3.5). Bottom rows: chemical abundances derived from MEGARA spectra (Sect. 4).(a)Based on only two stars.

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