Table 3.
Effective temperature (Teff), surface gravity (logg), metallicity ([Fe/H]), and microturbulence velocity (ξ) of the objects with a determined orbit.
| Name | Type | Teff [K] | logg [dex] | [Fe/H] [dex] | ξ [km s−1] | Ref. | E(B − V) | L/L⊙ | M/M⊙ |
|---|---|---|---|---|---|---|---|---|---|
| BD-10°4311 | sgCH | 5858 ± 50 | 3.9 ± 0.3 | −0.65 ± 0.10 | 1.25 ± 0.07 | This work | 0.042 ± 0.015 | 1.99 ± 0.05 | 0.80 ± 0.10 |
| BD-18°255 | dBa | 6800 ± 400 | 4.3 ± 0.3 | −0.18 ± 0.05 | 2.4 ± 0.5 | L&B91 | 0.015 ± 0.005 | 4.2 ± 1.2 | 1.30 ± 0.15 |
| BD+18°5215 | dBa | 6452 ± 50 | 4.4 ± 0.4 | −0.50 ± 0.09 | 0.82 ± 0.09 | This work | 0.014 ± 0.007 | 1.86 ± 0.11 | 1.10 ± 0.10 |
| HD 15306 | dBa | 6898 ± 50 | 3.8 ± 0.2 | −0.40 ± 0.14 | 0.9 ± 0.3 | This work | 0.037 ± 0.007 | 8.7 ± 2.3 | 1.30 ± 0.10 |
| HD 22589 | gBa | 5672 ± 56 | 3.9 ± 0.2 | −0.07 ± 0.09 | 1.20 ± 0.04 | This work | 0.048 ± 0.008 | 6.9 ± 0.8 | 1.30 ± 0.10 |
| HD 24864 | dBa | 6337 ± 95 | 3.82 ± 0.18 | 0.0 ± 0.11 | 1.0 ± 1.0 | K+13 | 0.0 + 0.005 | 9.2 ± 0.6 | 1.38 ± 0.06 |
| HD 34654 | dBa | 6174 ± 50 | 4.4 ± 0.3 | −0.09 ± 0.07 | 1.36 ± 0.04 | This work | 0.012 ± 0.008 | 1.8 ± 0.3 | 1.19 ± 0.05 |
| HD 48565 | dBa | 6030 ± 100 | 3.8 ± 0.3 | −0.6 ± 0.3 | 1.3 ± 0.3 | K&G14 | 0.018 ± 0.010 | 2.8 ± 0.3 | 0.92 ± 0.05 |
| HD 50264 | dBa | 5800 ± 100 | 4.2 ± 0.2 | −0.34 ± 0.08 | 1.0 ± 0.3 | P&J03 | 0.002 ± 0.010 | 0.89 ± 0.08 | 0.90 ± 0.10 |
| HD 76225 | dBa | 6340 ± 50 | 3.9 ± 0.2 | −0.37 ± 0.08 | 1.30 ± 0.06 | This work | 0.053 ± 0.010 | 5.9 ± 0.7 | 1.21 ± 0.06 |
| HD 87080 | sgCH | 5483 ± 50 | 3.6 ± 0.3 | −0.60 ± 0.08 | 1.20 ± 0.04 | This work | 0.028 ± 0.012 | 12.5 ± 0.8 | 1.6 ± 0.2 |
| HD 89948 | sgCH | 6000 ± 400 | 4.0 ± 0.3 | −0.13 ± 0.05 | 1.8 ± 0.5 | L&B91 | 0.0 ± 0.003 | 1.36 ± 0.07 | 0.95 ± 0.08 |
| HD 95241 | dBa | 5837 ± 50 | 3.6 ± 0.2 | −0.37 ± 0.07 | 1.36 ± 0.04 | This work | 0.0 + 0.008 | 7.8 ± 0.8 | 1.30 ± 0.10 |
| HD 98991 | dBa | 6388 ± 50 | 2.7 ± 0.4 | −0.44 ± 0.08 | 0.07(1) | This work | 0.0 + 0.014 | 14.7 ± 1.0 | 1.45 ± 0.08 |
| HD 106191 | dBa | 5946 ± 50 | 4.3 ± 0.4 | −0.29 ± 0.10 | 1.21 ± 0.06 | This work | 0.010 ± 0.010 | 2.0 ± 0.2 | 0.95 ± 0.05 |
| HD 107574 | dBa | 6340 ± 100 | 3.6 ± 0.5 | −0.80 ± 0.25 | 1.8 ± 0.3 | N+94 | 0.0 + 0.005 | 5.6 ± 0.2 | 1.11 ± 0.05 |
| HD 120620 | gBa | 4831 ± 50 | 3.0 ± 0.3 | −0.29 ± 0.10 | 1.11 ± 0.05 | This work | 0.055 ± 0.013 | 12.2 ± 1.6 | 1.2 ± 0.2 |
| HD 123585 | sgCH | 6047 ± 100 | 3.5 ± 0.5 | −0.50 ± 0.25 | 1.8 ± 0.3 | N+94 | 0.054 ± 0.012 | 3.5 ± 1.0 | 1.00 ± 0.10 |
| HD 127392 | sgCH | 5600 ± 300 | 3.9 ± 0.3 | −0.52 ± 0.05 | 2.6 ± 0.5 | L&B91 | 0.011 ± 0.011 | 0.98 ± 0.13 | 0.8 ± 0.3 |
| HD 141804 | sgCH | 6000 ± 400 | 3.5 ± 0.3 | −0.41 ± 0.05 | 1.7 ± 0.5 | L&B91 | 0.0 + 0.003 | 1.77 ± 0.07 | 0.9 ± 0.2 |
| HD 147609 | dBa | 6411 ± 50 | 3.9 ± 0.5 | −0.23 ± 0.09 | 1.26 ± 0.07 | This work | 0.044 ± 0.007 | 10.2 ± 1.3 | 1.40 ± 0.10 |
| HD 150862 | sgCH | 6182 ± 50 | 4.1 ± 0.3 | −0.33 ± 0.08 | 0.94 ± 0.06 | This work | 0.006 ± 0.006 | 2.2 ± 0.2 | 1.04 ± 0.05 |
| HD 182274 | sgCH | 6327 ± 50 | 4.3 ± 0.2 | −0.32 ± 0.09 | 1.05 ± 0.06 | This work | 0.012 ± 0.007 | 2.06 ± 0.14 | 1.09 ± 0.05 |
| HD 207585 | sgCH | 5400 ± 300 | 3.3 ± 0.3 | −0.57 ± 0.05 | 1.8 ± 0.5 | L&B91 | 0.0 + 0.003 | 3.8 ± 0.8 | 0.96 ± 0.15 |
| HD 216219 | gBa | 5900 ± 50 | 3.6 ± 0.3 | −0.17 ± 0.08 | 1.42 ± 0.04 | This work | 0.042 ± 0.009 | 9.9 ± 0.8 | 1.45 ± 0.10 |
| HD 221531 | dBa | 6460 ± 100 | 4.2 ± 0.5 | −0.30 ± 0.25 | 2.4 ± 0.3 | N+94 | 0.0 + 0.004 | 4.7 ± 1.4 | 1.20 ± 0.10 |
Notes. Column 7 gives the reference of the adopted stellar parameters when no HERMES spectra were available. Column 8 gives the line-of-sight extinction, and Cols. 9 and 10 list the derived luminosities and masses.
(1)Uncertain value due to the low signal-to-noise ratio of the spectrum around Fe lines.
References. For the spectroscopic stellar parameters:
L&B91: Luck & Bond (1991); K+13: Kordopatis et al. (2013); K&G14: Karinkuzhi & Goswami (2014); P&J03: Pereira & Junqueira (2003); N+94: North et al. (1994).
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