Table 4
Results for the stellar parameters, for the DMA (upper portion) and SAT (lower portion) subsamples.
Tex (K) | log g | [FeI/H] | [FeII/H] | ξ (km s-1) | BC(V) | M V | M bol | L/L⊙ | R/R⊙ | M/M⊙ | D (pc) | [Ba/Eu] | Class | Var. |
|
||||||||||||||
DMA subsample | ||||||||||||||
|
||||||||||||||
BS 15621-047 | ||||||||||||||
4750 | 1.48 | –2.29 | –2.35 | 1.05 | –0.384 | –1.38 | –1.76 | 02.85 | 29.73 | 0.96 | 9700 | –0.49 | r | B |
70 | 0.09 | 0.07 | 0.09 | 0.05 | 0.025 | 0.21 | 0.20 | 76.37 | 2.97 | 0.09 | 1188 | |||
|
||||||||||||||
BS 16033-081 | ||||||||||||||
5020 | 1.84 | –2.20 | –2.07 | 1.2 | –0.297 | –0.61 | –0.91 | 82.92 | 17.94 | 0.80 | 5620 | –1.31 | r | B |
50 | 0.07 | 0.05 | 0.07 | 0.1 | 0.014 | 0.13 | 0.12 | 21.33 | 1.12 | 0.00 | 542 | |||
|
||||||||||||||
BS 16077-077 | ||||||||||||||
5900 | 3.19 | –2.05 | –2.00 | 1.00 | –0.164 | 1.76 | 1.59 | 18.29 | 4.11 | 0.95 | 2344 | 0.76 | s | |
50 | 0.08 | 0.05 | 0.09 | 0.20 | 0.007 | 0.20 | 0.20 | 3.45 | 0.41 | 0.09 | 279 | |||
|
||||||||||||||
BS 16082-129 | ||||||||||||||
5080 | 1.98 | –2.65 | –2.59 | 1.30 | –0.298 | –0.26 | –0.56 | 32.80 | 14.92 | 0.77 | 5200 | ... | no?r? | |
50 | 0.11 | 0.06 | 0.08 | 0.05 | 0.014 | 0.27 | 0.27 | 33.05 | 1.89 | 0.13 | 773 | |||
|
||||||||||||||
BS 16543-097 | ||||||||||||||
5220 | 2.54 | –2.48 | –2.36 | 1.85 | –0.264 | 1.00 | 0.73 | 40.41 | 7.80 | 0.77 | 1970 | –0.49 | r | |
50 | 0.10 | 0.06 | 0.08 | 0.10 | 0.012 | 0.16 | 0.16 | 6.10 | 0.61 | 0.05 | 225 | |||
|
||||||||||||||
BS 16929-005 | ||||||||||||||
5250 | 3.10 | –3.15 | –3.02 | 0.90 | –0.288 | 2.40 | 2.11 | 11.39 | 4.09 | 0.77 | 1670 | –0.74 | r | |
50 | 0.09 | 0.06 | 0.09 | 0.10 | 0.010 | 0.22 | 0.22 | 2.29 | 0.42 | 0.10 | 207 | |||
|
||||||||||||||
CS 22949-008 | ||||||||||||||
6000 | 3.74 | –2.45 | –2.61 | 1.5 | –0.181 | 3.32 | 3.14 | 4.40 | 1.95 | 0.76 | 1430 | ... | s?rs? | |
50 | 0.07 | 0.03 | 0.09 | 0.1 | 0.002 | 0.15 | 0.15 | 0.61 | 0.14 | 0.05 | 143 | |||
|
||||||||||||||
CS 29503-010 | ||||||||||||||
6050 | 3.66 | –1.69 | –1.70 | 1.6 | –0.135 | 2.91 | 2.77 | 6.17 | 2.27 | 0.86 | 1400 | 0.12 | rs | |
50 | 0.08 | 0.02 | 0.06 | 0.1 | 0.003 | 0.15 | 0.15 | 0.87 | 0.17 | 0.05 | 146 | |||
|
||||||||||||||
CS 29512-073 | ||||||||||||||
5560 | 3.44 | –2.06 | –1.88 | 1.1 | –0.195 | 2.78 | 2.58 | 7.35 | 2.93 | 0.86 | 1730 | 1.05 | s | |
50 | 0.07 | 0.02 | 0.04 | 0.1 | 0.006 | 0.12 | 0.12 | 0.85 | 0.18 | 0.02 | 160 | |||
|
||||||||||||||
CS 29526-110 | ||||||||||||||
6650 | 3.79 | –2.19 | –2.29 | 1.6 | –0.152 | 2.85 | 2.70 | 6.62 | 1.95 | 0.85 | 1170 | 0.01 | rs | B |
50 | 0.07 | 0.04 | 0.10 | 0.1 | 0.002 | 0.12 | 0.12 | 0.76 | 0.12 | 0.02 | 108 | |||
|
||||||||||||||
CS 29528-028 | ||||||||||||||
7100 | 4.27 | –2.12 | –2.17 | 1.2 | –0.155 | 3.81 | 3.65 | 2.75 | 1.10 | 0.81 | 1320 | 0.33 | rs | |
50 | 0.07 | 0.06 | 0.18 | 0.3 | 0.003 | 0.12 | 0.12 | 0.31 | 0.07 | 0.02 | 121 | |||
|
||||||||||||||
CS 31070-073 | ||||||||||||||
6190 | 3.86 | –2.55 | –2.64 | 1.5 | –0.181 | 3.43 | 3.25 | 3.99 | 1.74 | 0.80 | 1630 | –0.41 | r | |
50 | 0.07 | 0.03 | 0.08 | 0.1 | 0.001 | 0.12 | 0.12 | 0.46 | 0.11 | 0.02 | 150 | |||
|
||||||||||||||
SAT subsample | ||||||||||||||
|
||||||||||||||
Tex (K) | log g | [Fe/H] | ξ (km s-1) | [Ba/Eu] | Class | Var. | ||||||||
|
||||||||||||||
BS 16080-175 | ||||||||||||||
6240 ± 100 | 3.70 ± 0.1 | –1.86 ± 0.2 | 1.05 ± 0.1 | 0.5 | rs | |||||||||
|
||||||||||||||
BS 17436-058 | ||||||||||||||
5340 ± 100 | 2.20 ± 0.1 | –1.90 ± 0.2 | 2.70 ± 0.1 | 0.44 | rs | |||||||||
|
||||||||||||||
CS 22183-015 | ||||||||||||||
5470 ± 100 | 2.85 ± 0.1 | –2.85 ± 0.2 | 1.45 ± 0.1 | 0.52 | s?rs? | |||||||||
|
||||||||||||||
CS 22887-048 | ||||||||||||||
6500 ± 100 | 3.35 ± 0.1 | –1.70 ± 0.2 | 2.05 ± 0.1 | 0.51 | s?rs? | B | ||||||||
|
||||||||||||||
CS 22898-027 | ||||||||||||||
6240 ± 100 | 3.72 ± 0.1 | –2.30 ± 0.2 | 1.40 ± 0.1 | 0.35 | rs | |||||||||
|
||||||||||||||
CS 29502-092 | ||||||||||||||
4970 ± 100 | 1.70 ± 0.1 | –3.05 ± 0.2 | 1.85 ± 0.1 | –1.58 | r | |||||||||
|
Notes. For the DMA subsample, Tex is the excitation temperature, Mbol is the bolometric magnitude, L is the luminosity, R is the radii, M the mass, π the parallax. Uncertainties are shown in the second line. For [Fe/H], the uncertainties are the standard error of the mean abundance, excluding the effects of errors on atmosphere parameters. SAT did not use isochrones, so did not determine values for BC(V), MV, Mbol, L, R, M or D. The last column indicates whether the star is binary or not, according to Tsangarides (2005).
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