J/A+A/512/A41/table5 | Abundances of microlensed stars in the Bulge (Bensby+, 2010) Abundances and uncertainties for each star (13 rows) | Name==MOA-2009-BLG-493S |
Column | Value | Explain (UCD) | |
2recno | 2 | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) | |
Name | MOA-2009-BLG-493S | Star name (meta.id;meta.main) | |
[Fe/H] | -0.70 | [Sun] | Normalised abundance (phys.abund) |
e_[Fe/H] | 0.14 | [Sun] | Error in abundance ratio (stat.error;phys.abund.Fe) |
[O/Fe] | 0.43 | [Sun] | Normalised abundance (not NLTE corrected) (phys.abund) |
e_[O/Fe] | 0.51 | [Sun] | Error in abundance ratio (phys.abund) |
[Na/Fe] | 0.13 | [Sun] | Normalised abundance (phys.abund) |
e_[Na/Fe] | 0.07 | [Sun] | Error in abundance ratio (phys.abund) |
[Mg/Fe] | 0.37 | [Sun] | Normalised abundance (phys.abund) |
e_[Mg/Fe] | 0.10 | [Sun] | Error in abundance ratio (phys.abund) |
[Al/Fe] | 0.28 | [Sun] | Normalised abundance (phys.abund) |
e_[Al/Fe] | 0.08 | [Sun] | Error in abundance ratio (phys.abund) |
[Si/Fe] | 0.18 | [Sun] | Normalised abundance (phys.abund) |
e_[Si/Fe] | 0.19 | [Sun] | Error in abundance ratio (phys.abund) |
[Ca/Fe] | 0.17 | [Sun] | Normalised abundance (phys.abund) |
e_[Ca/Fe] | 0.30 | [Sun] | Error in abundance ratio (phys.abund) |
[Ti/Fe] | 0.34 | [Sun] | Normalised abundance (phys.abund) |
e_[Ti/Fe] | 0.08 | [Sun] | Error in abundance ratio (phys.abund) |
[Cr/Fe] | 0.01 | [Sun] | Normalised abundance (phys.abund) |
e_[Cr/Fe] | 0.10 | [Sun] | Error in abundance ratio (phys.abund) |
[Ni/Fe] | 0.04 | [Sun] | Normalised abundance (phys.abund) |
e_[Ni/Fe] | 0.17 | [Sun] | Error in abundance ratio (phys.abund) |
[Zn/Fe] | 0.25 | [Sun] | Normalised abundance (phys.abund) |
e_[Zn/Fe] | 0.38 | [Sun] | Error in abundance ratio (phys.abund) |
[Y/Fe] | [Sun] | Normalised abundance (phys.abund) | |
e_[Y/Fe] | [Sun] | Error in abundance ratio (phys.abund) | |
[Ba/Fe] | -0.07 | [Sun] | Normalised abundance (phys.abund) |
e_[Ba/Fe] | 0.18 | [Sun] | Error in abundance ratio (phys.abund) |
e_[O/H] | 0.38 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Na/H] | 0.09 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Mg/H] | 0.16 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Al/H] | 0.07 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Si/H] | 0.06 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Ca/H] | 0.43 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Ti/H] | 0.13 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Cr/H] | 0.07 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Ni/H] | 0.05 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Zn/H] | 0.26 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
e_[Y/H] | [Sun] | Error in abundance ratio (stat.error;phys.abund) | |
e_[Ba/H] | 0.18 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
n(Fe) | 80 | Number of Fe lines used (meta.number) | |
n(O) | 3 | Number of O lines used (meta.number) | |
n(Na) | 1 | Number of Na lines used (meta.number) | |
n(Mg) | 6 | Number of Mg lines used (meta.number) | |
n(Al) | 6 | Number of Al lines used (meta.number) | |
n(Si) | 19 | Number of Si lines used (meta.number) | |
n(Ca) | 10 | Number of Ca lines used (meta.number) | |
n(Ti) | 5 | Number of Ti lines used (meta.number) | |
n(Cr) | 2 | Number of Cr lines used (meta.number) | |
n(Ni) | 21 | Number of Ni lines used (meta.number) | |
n(Zn) | 1 | Number of Zn lines used (meta.number) | |
n(Y) | Number of Y lines used (meta.number) | ||
n(Ba) | 4 | Number of Ba lines used (meta.number) |