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Table 3

LTE atmospheric abundances of HD 216711 with the error estimates based on the internal scatter from the number of measured lines, n.

Ion HD 216711 VAS 20 VAS 87 Sun
log (N/Ntot) n log (N/Ntot)
C i −3.43 ± 0.04 5 −3.61
Na i −5.53 ± 0.13 2 −5.83 −5.68 −5.87
Mg i −4.46 ± 0.13 4 −4.63 −4.55 −4.44
Mg ii −4.42 ± 0.10 2 −4.44
Si i −4.59: 1 −4.58 −4.87 −4.53
Si ii −4.47 ± 0.10 5 −4.49 −4.53
Ca i −5.65 ± 0.12 11 −5.64 −5.71 −5.70
Ca ii −5.85 ± 0.13 2 −5.70
Sc ii −9.12 ± 0.08 4 −8.97 −9.16 −8.89
Ti ii −7.20 ± 0.10 6 −7.03 −7.14 −7.09
Cr i −6.86 ± 0.05 3 −6.37 −6.39 −6.40
Cr ii −6.38 ± 0.11 7 −6.44 −6.06 −6.40
Mn i −6.36 ± 0.23 3 −6.36 −6.44 −6.61
Fe i −4.62 ± 0.20 45 −4.55 −4.63 −4.54
Fe ii −4.61 ± 0.14 27 −4.52 −4.58 −4.54
Ni i −5.88 ± 0.11 3 −5.77 −5.83 −5.82
Sr ii −9.56: 1 −9.17
Y ii −9.60: 1 −9.94 −9.66 −9.83
Zr ii −9.10: 1 −9.46
Ba ii −9.52 ± 0.32 3 −9.29 −9.51 −9.86
T eff 8600 K 6380 K 6220 K 5777 K
log g 4.1 4.0 3.8 4.44

Notes.For comparison purpose, columns 4,5 and 6 list respectively the abundances obtained by Zwintz et al. (2013) for NGC 2264 VAS 20 and NGC 2264 VAS 87 and for the Sun (Asplund et al. 2009).

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