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Table 8

Best-fit stellar parameters of the stars in the sample and corresponding upper and lower 1σ uncertainties.

Star Teff log g v sin i ξ log v β fcl
(kK) (cm s−2) (km s−1) (km s−1) (M yr−1) (km s−1)
64066 38.02.5+4.0$38.0_{-2.5}^{+4.0}$ 3.320.12+0.26$3.32_{-0.12}^{+0.26}$ 17838+45$178_{-38}^{+45}$ 21.04.4+0.3$21.0_{-4.4}^{+0.3}$ 7.9+1.4$-7.9_{\downarrow}^{+1.4}$ 2000200+200$2000_{-200}^{+200}$ 0.95 5655+5$56_{-55}^{+5}$
A13 44.750.5+0.75$44.75_{-0.5}^{+0.75}$ 3.750.05+0.17$3.75_{-0.05}^{+0.17}$ 6510+25$65_{-10}^{+25}$ 20.40.6+0.9$20.4_{-0.6}^{+0.9}$ 6.810.15+0.10$-6.81_{-0.15}^{+0.10}$ 212575+50$2125_{-75}^{+50}$ 1.560.34+0.02$1.56_{-0.34}^{+0.02}$ 3011+11$30_{-11}^{+11}$
62024 38.752.5+1.5$38.75_{-2.5}^{+1.5}$ 3.840.4+0.16$3.84_{-0.4}^{+0.16}$ 16055+55$160_{-55}^{+55}$ 19.18.1+2.2$19.1_{-8.1}^{+2.2}$ 6.840.25+0.15$-6.84_{-0.25}^{+0.15}$ 1050200+120$1050_{-200}^{+120}$ 2.120.47+0.10$2.12_{-0.47}^{+0.10}$ 4523+16$45_{-23}^{+16}$
B2 37.51.5+2.2$37.5_{-1.5}^{+2.2}$ 3.720.16+0.18$3.72_{-0.16}^{+0.18}$ 10335+28$103_{-35}^{+28}$ 1.91.2+4.1$1.9_{-1.2}^{+4.1}$ 8.650.7+0.30$-8.65_{-0.7}^{+0.30}$ 1025400+650$1025_{-400}^{+650}$ 1.040.46+0.62$1.04_{-0.46}^{+0.62}$ 1311+48$13_{-11}^{+48}$
B11 33.250.75+0.25$33.25_{-0.75}^{+0.25}$ 3.540.08+0.06$3.54_{-0.08}^{+0.06}$ 13028+18$130_{-28}^{+18}$ 5.11.6+3.1$5.1_{-1.6}^{+3.1}$ 8.580.2+0.55$-8.58_{-0.2}^{+0.55}$ 1350120+25$1350_{-120}^{+25}$ 0.920.14+0.02$0.92_{-0.14}^{+0.02}$ 43+2$4_{-3}^{+2}$
A15 37.50.56+0.19$37.5_{-0.56}^{+0.19}$ 3.820.14+0.02$3.82_{-0.14}^{+0.02}$ 605+18$60_{-5}^{+18}$ 12.20.9+3.1$12.2_{-0.9}^{+3.1}$ 8.890.2+0.15$-8.89_{-0.2}^{+0.15}$ 1200120+75$1200_{-120}^{+75}$ 0.760.18+0.04$0.76_{-0.18}^{+0.04}$ 2112+19$21_{-12}^{+19}$
A11 33.251.0+1.5$33.25_{-1.0}^{+1.5}$ 3.460.14+0.46$3.46_{-0.14}^{+0.46}$ 15030+40$150_{-30}^{+40}$ 20.45.9+0.9$20.4_{-5.9}^{+0.9}$ 9.390.1+0.30$-9.39_{-0.1}^{+0.30}$ 1325200+400$1325_{-200}^{+400}$ 0.680.1+0.10$0.68_{-0.1}^{+0.10}$ 4134+20$41_{-34}^{+20}$
N20 30.750.25+1.5$30.75_{-0.25}^{+1.5}$ 3.50.02+0.28$3.5_{-0.02}^{+0.28}$ 18042+8$180_{-42}^{+8}$ 16.65.6+4.4$16.6_{-5.6}^{+4.4}$ 7.480.05+0.35$-7.48_{-0.05}^{+0.35}$ 160075+150$1600_{-75}^{+150}$ 0.90.16+0.48$0.9_{-0.16}^{+0.48}$ 4621+9$46_{-21}^{+9}$
N34 33.752.8+2.2$33.75_{-2.8}^{+2.2}$ 3.360.32+0.32$3.36_{-0.32}^{+0.32}$ 10352+25$103_{-52}^{+25}$ 3.22.5+15.0$3.2_{-2.5}^{+15.0}$ 7.30.2+1.2$-7.3_{-0.2}^{+1.2}$ 1725300+25$1725_{-300}^{+25}$ 1.91.1+0.0$1.9_{-1.1}^{+0.0}$ 1817+28$18_{-17}^{+28}$
S3 33.250.75+1.5$33.25_{-0.75}^{+1.5}$ 4.180.08+0.14$4.18_{-0.08}^{+0.14}$ 27844+16$278_{-44}^{+16}$ 4.80.9+5.0$4.8_{-0.9}^{+5.0}$ 9.21+0.3$-9.21_{\downarrow}^{+0.3}$ 25075+180$250_{-75}^{+180}$ 0.620.04+0.18$0.62_{-0.04}^{+0.18}$ 5751+4$57_{-51}^{+4}$
LP26 33.01.8+1.8$33.0_{-1.8}^{+1.8}$ 4.220.16+0.18$4.22_{-0.16}^{+0.18}$ 14540+65$145_{-40}^{+65}$ 1.00.3+5.0$1.0_{-0.3}^{+5.0}$ 9.8+1.4$-9.8_{\downarrow}^{+1.4}$ 800720+1400$800_{-720}^{+1400}$ 0.660.08+0.96$0.66_{-0.08}^{+0.96}$ 2322+38$23_{-22}^{+38}$

Notes. Down arrows indicate upper limits.

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