J0251-0006
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6062+-174 | log g : 3.85+-0.05 | vturb : 1.90+-0.21 |
| 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 | ... | 2.10+-0.22 | 2.10+-0.22 | -1.16+-0.22 | 1.81+-0.22 | 2.10+-0.22 | Li I |
| C | ... | <1.51 | <6.97 | <-1.46 | <1.51 | <6.97 | C | |
| Na I | 2 | ... | -0.30+-0.11 | 2.97+-0.11 | -3.27+-0.11 | -0.30+-0.11 | 2.97+-0.11 | Na I |
| Mg I | 3 | ... | 0.25+-0.20 | 4.88+-0.20 | -2.72+-0.20 | 0.25+-0.20 | 4.88+-0.20 | Mg I |
| Ca I | 3 | ... | 0.36+-0.16 | 3.73+-0.16 | -2.61+-0.16 | 0.36+-0.16 | 3.73+-0.16 | Ca I |
| Sc II | 1 | ... | 0.40+-0.16 | 0.58+-0.16 | -2.57+-0.16 | 0.40+-0.16 | 0.58+-0.16 | Sc II |
| Ti II | 7 | ... | 0.67+-0.17 | 2.65+-0.17 | -2.30+-0.17 | 0.67+-0.17 | 2.65+-0.17 | Ti II |
| Cr I | 3 | ... | -0.06+-0.11 | 2.61+-0.11 | -3.03+-0.11 | -0.06+-0.11 | 2.61+-0.11 | Cr I |
| Fe I | 23 | ... | 0.00+-0.15 | 4.53+-0.15 | -2.97+-0.15 | 0.00+-0.15 | 4.53+-0.15 | Fe I |
| Fe II | 4 | ... | 0.11+-0.22 | 4.64+-0.22 | -2.86+-0.22 | 0.11+-0.22 | 4.64+-0.22 | Fe II |
| Sr II | 2 | ... | 0.35+-0.14 | 0.25+-0.14 | -2.62+-0.14 | 0.35+-0.14 | 0.25+-0.14 | Sr II |
| Ba II | 2 | ... | 0.44+-0.13 | -0.35+-0.13 | -2.53+-0.13 | 0.44+-0.13 | -0.35+-0.13 | Ba II |
| Right Ascension : 02 51 50.28 | Declination : -00 06 36.50 | 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 | 26.0 | N/A | -46.2 |