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Table 2

Stellar parameters and Be and Li abundances from the literature (García López & Pérez de Taoro 1998; Santos et al. 2002, 2004c; Sousa et al. 2008): stars hosting planets.

Name T eff log g [Fe/H] Massa SpTb LCc log N(Be) log N(Li) [O/H]d Agee
[K] [cm s-2] M [dex] [dex] [dex] Gyr

BD–103166 5320 4.38 0.33  − K0V V  < 0.5 5.39
HD 6434 5835 4.6 –0.52 0.82 G2/G3V V 1.08  < 0.85  −0.18 ± 0.1 13.3
HD 9826 6212 4.26 0.13 1.30 F8V V 1.05 2.55 0.22 ± 0.12
HD 10647 6143 4.48 –0.03 1.20 F9V V 1.19 2.8  −0.06 ± 0.09 4.8
HD 10697 5641 4.05 0.14 1.22 G5IV IV 1.31 1. 96 1.17
HD 12661 5702 4.33 0.36 1.05 K0V V 1.13  < 0.98 7.05
HD 13445 5163 4.52 –0.24 0.70 K1V V  < 0.4  < –0.12  −0.25 ± 0.12
HD 16141 5801 4.22 0.15 1.06 G5IV V 1.17 1.11 0.19 ± 0.10 11.2
HD 17051 6252 4.61 0.26 1.26 F9VFe+03 V 1.03 2.66 0.33 ± 0.11 1.47
HD 19994 6190 4.19 0.24 1.37 F8V V 0.93 1.99 0.31 ± 0.12 4.7
HD 22049 5073 4.43 –0.13 0.85 K2V V 0.77  < 0.25  −0.23 ± 0.10
HD 27442 4825 3.55 0.39  − K2III III  < 0.3  < –0.47 0.07 ± 0.14
HD 38529 5674 3.94 0.4 1.60 G4V IV  < –0.1  < 0.61 5.09
HD 46375 5268 4.41 0.2 0.82 K1IV V  < 0.8  < –0.02 0.04 ± 0.10 16.4
HD 52265 6103 4.28 0.23 1.20 G0III-IV V 1.25 2.88 0.21 ± 0.10 3.8
HD 69830 5410 4.38 –0.03 0.82 K0V V 0.79  < 0.47
HD 75289 6143 4.42 0.28 1.24 F9VFe+03 V 1.36 2.85 0.22 ± 0.11 4.0
HD 75732Af 5150 4.15 0.29 0.87 G8V IV 0.55  < 0.04
HD 82943 6016 4.46 0.3 1.15 F9VFe+05 V 1.27 2.51 0.29 ± 0.11 3.5
HD 83443 5454 4.33 0.35 0.95 K0V V  < 0.7  < 0.52 0.12 ± 0.13 2.94
HD 92788 5821 4.45 0.32 1.03 G5 V 1.19 1.34 9.6
HD 95128 5954 4.44 0.06 1.07 G1V V 1.23 1.83
HD 108147 6248 4.49 0.2 1.26 F8VH+04 V 0.99 2.33 1.98
HD 114762 5884 4.22 –0.7 0.81 F9V V 0.82 2.2 11.8
HD 117176 5560 4.07 –0.06 0.93 G5V IV 0.86 1.88
HD 120136 6339 4.19 0.23 1.33 F6IV V  < 0.25
HD 121504 6075 4.64 0.16 1.13 G2V V 1.33 2.65 1.62
HD 130322 5392 4.48 0.03 0.88 K0III V 0.95  < 0.13 1.24
HD 134987 5776 4.36 0.3 1.03 G5V V 1.22  < 0.74 11.1
HD 143761 5853 4.41 –0.21 0.95 G0Va V 1.11 1.46  −0.09 ± 0.08
HD 145675 5311 4.42 0.43 0.90 K0V V  < 0.65  < 0.03 7.6
HD 168443 5617 4.22 0.06 0.96 G6V V 1.11  < 0.78 10.6
HD 169830 6299 4.1 0.21 1.42 F7V V  < –0.4  < 1.16 0.22 ± 0.12 2.3
HD 179949 6260 4.43 0.22 1.28 F8.5V V 1.08 2.65 0.26 ± 0.11 2.05
HD 186427f 5700 4.35 0.06 0.99 G3V V 1.3 0.46
HD 187123 5845 4.42 0.13 1.04 G5 V 1.08 1.21 7.3
HD 192263 4947 4.51 –0.02 0.69 K2V V  < 0.9  < –0.39  −0.17 ±  0.09 0.57
HD 195019 5842 4.32 0.08 1.06 G3IV-V V 1.15 1.47 10.6
HD 202206 5752 4.5 0.35 1.04 G6V V 1.04 1.04 0.20 ± 0.09 2.04
HD 209458 6117 4.48 0.02 1.15 G0V V 1.24 2.7 0.03 ± 0.07 6.6
HD 210277 5532 4.29 0.19 0.90 G0V V 0.91  < 0.3 0.13 ± 0.12 6.93
HD 217014 5804 4.42 0.2 1.05 G5V V 1.02 1.3  −0.06 ± 0.11
HD 217107 5646 4.31 0.37 1.02 G8IV V 0.96  < 0.4 0.29 ± 0.13 7.32
HD 222582 5843 4.45 0.05 0.97 G5 V 1.14  < 0.59 0.09 ± 0.08 11.1

Notes. 

(a)

Values taken from Sousa et al. (2008) and Santos et al. (2004a).

(b)

Values taken from SIMBAD.

(c)

Luminosity class assigned by comparing the stellar parameters with isochrones from Girardi et al. (2000).

(d)

Values taken from Ecuvillon et al. (2006).

(e)

Values taken from Saffe et al. (2005).

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