J0422+1808
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 4514+-32 | log g : 1.29+-0.19 | vturb : 2.08+-0.19 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| C | ... | <0.01 | <4.38 | <-4.05 | <0.01 | <4.38 | C | |
| Na I | 2 | ... | -0.15+-0.11 | 2.03+-0.11 | -4.21+-0.11 | -0.15+-0.11 | 2.03+-0.11 | Na I |
| Mg I | 4 | ... | 0.54+-0.14 | 4.08+-0.14 | -3.52+-0.14 | 0.54+-0.14 | 4.08+-0.14 | Mg I |
| Ca I | 6 | ... | 0.55+-0.16 | 2.83+-0.16 | -3.51+-0.16 | 0.55+-0.16 | 2.83+-0.16 | Ca I |
| Sc II | 1 | ... | -0.78+-0.18 | -1.69+-0.18 | -4.84+-0.18 | -0.78+-0.18 | -1.69+-0.18 | Sc II |
| Ti II | 12 | ... | 0.61+-0.13 | 1.50+-0.13 | -3.45+-0.13 | 0.61+-0.13 | 1.50+-0.13 | Ti II |
| Cr I | 3 | ... | -0.45+-0.10 | 1.13+-0.10 | -4.51+-0.10 | -0.45+-0.10 | 1.13+-0.10 | Cr I |
| Fe I | 40 | ... | 0.00+-0.16 | 3.44+-0.16 | -4.06+-0.16 | 0.00+-0.16 | 3.44+-0.16 | Fe I |
| Fe II | 3 | ... | 0.26+-0.23 | 3.70+-0.23 | -3.80+-0.23 | 0.26+-0.23 | 3.70+-0.23 | Fe II |
| Ni I | 1 | ... | -0.37+-0.16 | 1.79+-0.16 | -4.43+-0.16 | -0.37+-0.16 | 1.79+-0.16 | Ni I |
| Ba II | 3 | ... | -0.71+-0.19 | -2.59+-0.19 | -4.77+-0.19 | -0.71+-0.19 | -2.59+-0.19 | Ba II |
| Right Ascension : 04 22 45.27 | Declination : +18 08 24.35 | 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 | 20.4 | N/A | 76.2 |