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Table 3:

Atmospheric parameters and C, N, O abundances.

Star
$T\rm {_{eff}}$ (K) $\log g$ $\xi$ (km s-1) [M/H] C N O
Late-R stars

HIP 35 810
3300 0.0 2.8 -0.38  8.40  7.30a 8.35
HIP 36 623 3300 0.0 2.1 -0.27  8.35 7.70 8.31
HIP 91 929 3300 0.0 2.5 0.00  8.68  7.78a 8.66
HIP 108 205 2500 0.0 2.3 0.00  8.67  7.78a 8.66
HIP 109 158 2500 0.0 2.5 -0.02  8.68  7.78a 8.66
Early-R stars

HIP 39 118
4250 2.0 1.8 -0.29  8.77 8.00 <9.05b
HIP 44 812 3950 1.5 3.0 -0.03  8.75 8.70 8.66
HIP 53 832 4500 2.5 2.3 -0.77  8.08 8.10 8.06
HIP 58 786 4250 2.0 2.2 -0.29  8.63 7.60 8.47
HIP 62 944 4300 2.4 2.0 0.12  8.80 8.30  9.05b
HIP 69 089 4750 1.5 2.0 -0.17  8.40 8.40 8.46
HIP 74 826 4750 2.0 1.5 -0.30  8.43 8.18 8.36
HIP 82 184 4500 2.0 3.0 -0.15  8.42 8.25 8.51
HIP 84 266 4750 2.0 2.4 -0.10  8.78 8.40 8.56
HIP 85 750 3800 1.2 2.0 -0.48  8.38 7.98 8.36
HIP 86 927 4700 2.4 2.3 -0.05  8.47 7.98 8.66
HIP 87 603 4100 2.0 2.3 -0.52  8.60 7.68 8.36
HIP 88 887 3950 1.5 3.0 -0.09  8.80 8.70 8.66
HIP 94 049 4100 2.0 2.3 -0.62  8.48 7.98 8.36
HIP 95 422 3950 2.0 3.0 -0.26  8.73  7.78a 8.36
HIP 98 223 3800 1.5 1.9 -0.79  8.05 7.10 7.97
HIP 113 150 4500 2.0 2.4 -0.47  8.85  7.60a 8.36

a N abundance scaled with the stellar metallicity.
b O abundance derived from the $\lambda $ 6300.3 Å [O I] line using the atomic line parameters from Caffau et al. (2008).

Source LaTeX | All tables | In the text

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