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Table 3

Stellar parameters, determined in the present study.

HD T eff log g(1) log g(2)  [Fe/H]  vsini Object type R x Ref log A(Li) Class

166 5514 4.6 4.6 0.16 4.0 BY –4.31 –4.33 2.24 A
1835 5790 4.5 ... 0.13 6.51 BY –4.58 –4.44 W04 2.45 A
3651 5277 4.5 4.5 0.15 0.0 V –6.07 –5.02 W04  <–0.52 wA
4256 5020 4.3 4.3 0.08 1.5 ... ... ...  <–0.40 ...
4628 4905 4.6 ... –0.21 1.5 ... –5.93 –4.85 H96, B95  <–0.45 wA
4635 5103 4.4 4.4 0.07 1.4 ... ... –4.67 W04  <0.15 A
4913 4342 4.4 ... 0.05 2.15 ... ... ...  <–0.90 ...
6660 4759 4.6 ... 0.08 2.5 ... ... ...  <–0.50 ...
7590 5962 4.4 4.4 –0.10 6.7 BY –4.69 –4.53 W04 2.73 A
7924 5165 4.4 4.4 –0.22 1.1 ... –5.71 –4.83 W04  <–0.30 wA
... ... ... ... ... ... ... ... ... ... ... ...

Notes. log g(1): spectroscopic, log g(2): astrometric, object type from SIMBAD, Rx adopted from the ROSAT catalogues or estimated from the ROSAT archive data, indices retrieved from different sources, the measured Li abundance, and the class of activity. The values, taken from Wright et al. (2004) are marked by W04; from Henri et al. (1996) – marked by H96; from Hall et al. (2007) – by H07; from Baliunas et al. (1995) – by B95, from Maldonado et al. (2010) – by M10. The stars with weak levels of the solar-type activity are marked by wA; the stars with high levels of the solar-type activity are marked by A in the last column.

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