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Table 3.

Stellar parameters and abundance ratios of stars.

Star Teff (K) log g [M/H] A(Li) C/O 12C/13C 14N/15N 16O/17O [F/M] [〈s〉/M]
Case 63 3000 0.0 −0.10 −2.00 1.05 52 1250 580 0.15 0.32
HD 292921 4000 1.5 −0.20 −0.40 0.63 35 0.20
IRAS 20540+5049 3200 0.0 0.10 0.66 57 980 0.00 0.30
Case 473 3100 0.0 0.00 −1.00 1.07 58 670 0.30 <0.50
2MASS J20560894+5059071 3400 0.0 −0.15 −1.00 0.58 30 0.08
Case 121 3300 0.0 −0.20 −1.00 1.07 55 >1000 1000 −0.10 0.20
Case 588 3000 0.0 −1.00 −0.60 1.41 60 800 1.00
DH Mon 2600 0.0 −0.30 0.60 1.06 10 200−500 0.00
IRAS 19582+2907 3050 0.0 0.00 −0.50 1.04 50 0.60
HD 11800 4100 1.0 0.10 0.90 0.35 28 700 −0.05 0.00
[D75b] Star30 3500 0.7 −0.10 −0.80 0.79 33 515 0.17 0.50
BD +60 2534 4000 0.7 0.10 0.15 0.54 25 500 0.07 0.10
MSB 75 3000 0.0 −0.25 −0.60 1.05 35 >700 650 −0.10 0.40
C* 908 3200 0.0 −0.30 0.00 1.07 50 1000 0.25
CSS 0291 3500 0.8 −0.20 −0.70 0.64 30 0.20
V493 Mon 2200 0.0 −0.50 <1.5 <25

Notes. The abundance of Li is given in the usual scale A(Li) = log (N(Li)/N(H)) + 12. An ellipsis (…) means that the corresponding spectral range was not accessible for the star or that we could not determine the specific abundance feature. See text for the typical uncertainty in the values of each column.

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