J1358+1257
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6540+-32 | log g : 2.59+-0.05 | vturb : 2.26+-0.29 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| C | ... | <1.50 | <7.55 | <-0.88 | <1.50 | <7.55 | C | |
| Na I | 2 | ... | -0.12+-0.13 | 3.74+-0.13 | -2.50+-0.13 | -0.12+-0.13 | 3.74+-0.13 | Na I |
| Mg I | 2 | ... | 0.78+-0.19 | 6.00+-0.19 | -1.60+-0.19 | 0.78+-0.19 | 6.00+-0.19 | Mg I |
| Ca I | 3 | ... | 0.39+-0.45 | 4.35+-0.45 | -1.99+-0.45 | 0.39+-0.45 | 4.35+-0.45 | Ca I |
| Sc II | 5 | ... | 0.34+-0.13 | 1.11+-0.13 | -2.04+-0.13 | 0.34+-0.13 | 1.11+-0.13 | Sc II |
| Ti II | 18 | ... | 0.34+-0.17 | 2.91+-0.17 | -2.04+-0.17 | 0.34+-0.17 | 2.91+-0.17 | Ti II |
| Cr I | 4 | ... | -0.15+-0.17 | 3.11+-0.17 | -2.53+-0.17 | -0.15+-0.17 | 3.11+-0.17 | Cr I |
| Fe I | 31 | ... | 0.00+-0.17 | 5.12+-0.17 | -2.38+-0.17 | 0.00+-0.17 | 5.12+-0.17 | Fe I |
| Fe II | 9 | ... | -0.06+-0.21 | 5.06+-0.21 | -2.44+-0.21 | -0.06+-0.21 | 5.06+-0.21 | Fe II |
| Sr II | 2 | ... | 1.16+-0.25 | 1.65+-0.25 | -1.22+-0.25 | 1.16+-0.25 | 1.65+-0.25 | Sr II |
| Y II | 2 | ... | 0.01+-0.12 | -0.16+-0.12 | -2.37+-0.12 | 0.01+-0.12 | -0.16+-0.12 | Y II |
| Right Ascension : 13 58 46.34 | Declination : +12 57 06.46 | 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 | 45.3 | N/A | 163.1 |