J0127-0016
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6326+-90 | log g : 4.25+-0.04 | vturb : 1.96+-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 |
| C | ... | <1.30 | <6.85 | <-1.58 | <1.30 | <6.85 | C | |
| Na I | 2 | ... | -0.29+-0.13 | 3.07+-0.13 | -3.17+-0.13 | -0.29+-0.13 | 3.07+-0.13 | Na I |
| Mg I | 4 | ... | 0.18+-0.05 | 4.90+-0.05 | -2.70+-0.05 | 0.18+-0.05 | 4.90+-0.05 | Mg I |
| Ca I | 3 | ... | 0.48+-0.14 | 3.94+-0.14 | -2.40+-0.14 | 0.48+-0.14 | 3.94+-0.14 | Ca I |
| Sc II | 1 | ... | 0.33+-0.18 | 0.60+-0.18 | -2.55+-0.18 | 0.33+-0.18 | 0.60+-0.18 | Sc II |
| Ti II | 9 | ... | 0.51+-0.16 | 2.58+-0.16 | -2.37+-0.16 | 0.51+-0.16 | 2.58+-0.16 | Ti II |
| Cr I | 3 | ... | -0.10+-0.11 | 2.66+-0.11 | -2.98+-0.11 | -0.10+-0.11 | 2.66+-0.11 | Cr I |
| Fe I | 25 | ... | 0.00+-0.18 | 4.62+-0.18 | -2.88+-0.18 | 0.00+-0.18 | 4.62+-0.18 | Fe I |
| Fe II | 3 | ... | 0.14+-0.23 | 4.76+-0.23 | -2.74+-0.23 | 0.14+-0.23 | 4.76+-0.23 | Fe II |
| Sr II | 2 | ... | 0.09+-0.14 | 0.08+-0.14 | -2.79+-0.14 | 0.09+-0.14 | 0.08+-0.14 | Sr II |
| Right Ascension : 01 27 52.56 | Declination : -00 16 16.25 | 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 | 24.8 | N/A | -71.7 |