J1131+1329
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 5740+-123 | log g : 3.70+-0.06 | vturb : 0.65+-0.30 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Li I | 1 | ... | 2.12+-0.20 | 2.12+-0.20 | -1.14+-0.20 | 1.19+-0.20 | 2.12+-0.20 | Li I |
| C | 1 | ... | 1.01+-0.24 | 7.11+-0.24 | -1.32+-0.24 | 1.01+-0.24 | 7.11+-0.24 | C |
| Na I | 2 | ... | -0.25+-0.14 | 3.66+-0.14 | -2.58+-0.14 | -0.25+-0.14 | 3.66+-0.14 | Na I |
| Mg I | 4 | ... | 0.12+-0.11 | 5.39+-0.11 | -2.21+-0.11 | 0.12+-0.11 | 5.39+-0.11 | Mg I |
| Ca I | 9 | ... | 0.32+-0.16 | 4.33+-0.16 | -2.01+-0.16 | 0.32+-0.16 | 4.33+-0.16 | Ca I |
| Sc II | 1 | ... | 0.54+-0.20 | 1.36+-0.20 | -1.79+-0.20 | 0.54+-0.20 | 1.36+-0.20 | Sc II |
| Ti II | 10 | ... | 0.47+-0.13 | 3.09+-0.13 | -1.86+-0.13 | 0.47+-0.13 | 3.09+-0.13 | Ti II |
| Cr I | 3 | ... | 0.61+-0.14 | 3.92+-0.14 | -1.72+-0.14 | 0.61+-0.14 | 3.92+-0.14 | Cr I |
| Fe I | 55 | ... | 0.00+-0.19 | 5.17+-0.19 | -2.33+-0.19 | 0.00+-0.19 | 5.17+-0.19 | Fe I |
| Fe II | 4 | ... | 0.08+-0.15 | 5.25+-0.15 | -2.25+-0.15 | 0.08+-0.15 | 5.25+-0.15 | Fe II |
| Ni I | 1 | ... | -0.06+-0.19 | 3.83+-0.19 | -2.39+-0.19 | -0.06+-0.19 | 3.83+-0.19 | Ni I |
| Sr II | 2 | ... | 0.70+-0.14 | 1.24+-0.14 | -1.63+-0.14 | 0.70+-0.14 | 1.24+-0.14 | Sr II |
| Ba II | 3 | ... | -0.27+-0.15 | -0.42+-0.15 | -2.60+-0.15 | -0.27+-0.15 | -0.42+-0.15 | Ba II |
| Right Ascension : 11 31 37.07 | Declination : +13 29 27.36 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| N/A | N/A | SUBARUHDS | 36000 | 17.1 | N/A | 88.1 |