J0854+1405
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6065+-92 | log g : 4.39+-0.03 | vturb : 2.17+-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 | ... | 2.13+-0.16 | 2.13+-0.16 | -1.13+-0.16 | 1.91+-0.16 | 2.13+-0.16 | Li I |
| C | ... | <1.40 | <6.78 | <-1.65 | <1.39 | <6.78 | C | |
| Na I | 2 | ... | -0.27+-0.10 | 2.92+-0.10 | -3.32+-0.10 | -0.28+-0.10 | 2.92+-0.10 | Na I |
| Mg I | 3 | ... | 0.43+-0.15 | 4.98+-0.15 | -2.62+-0.15 | 0.42+-0.15 | 4.98+-0.15 | Mg I |
| Ca I | 2 | ... | 0.33+-0.25 | 3.62+-0.25 | -2.72+-0.25 | 0.32+-0.25 | 3.62+-0.25 | Ca I |
| Sc II | 1 | ... | 0.35+-0.14 | 0.45+-0.14 | -2.70+-0.14 | 0.34+-0.14 | 0.45+-0.14 | Sc II |
| Ti II | 3 | ... | 0.43+-0.24 | 2.33+-0.24 | -2.62+-0.24 | 0.42+-0.24 | 2.33+-0.24 | Ti II |
| Cr I | 1 | ... | -0.09+-0.13 | 2.50+-0.13 | -3.14+-0.13 | -0.10+-0.13 | 2.50+-0.13 | Cr I |
| Fe I | 20 | ... | 0.01+-0.13 | 4.46+-0.13 | -3.04+-0.13 | 0.01+-0.13 | 4.46+-0.13 | Fe I |
| Fe II | 1 | ... | -0.16+-0.07 | 4.29+-0.07 | -3.21+-0.07 | -0.16+-0.07 | 4.29+-0.07 | Fe II |
| Sr II | 2 | ... | 0.05+-0.16 | -0.13+-0.16 | -3.00+-0.16 | 0.04+-0.16 | -0.13+-0.16 | Sr II |
| Right Ascension : 08 54 18.13 | Declination : +14 05 03.47 | 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 | 15.9 | N/A | 241.1 |