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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