J0357+3243
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 5427+-112 | log g : 3.61+-0.04 | vturb : 0.45+-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 | ... | 1.97+-0.18 | 1.97+-0.18 | -1.29+-0.18 | 1.40+-0.18 | 1.97+-0.18 | Li I |
| Na I | 2 | ... | -0.29+-0.12 | 3.27+-0.12 | -2.97+-0.12 | -0.28+-0.12 | 3.27+-0.12 | Na I |
| Mg I | 3 | ... | 0.17+-0.12 | 5.09+-0.12 | -2.51+-0.12 | 0.18+-0.12 | 5.09+-0.12 | Mg I |
| Ca I | 6 | ... | 0.23+-0.14 | 3.89+-0.14 | -2.45+-0.14 | 0.24+-0.14 | 3.89+-0.14 | Ca I |
| Ti II | 9 | ... | 0.42+-0.19 | 2.69+-0.19 | -2.26+-0.19 | 0.43+-0.19 | 2.69+-0.19 | Ti II |
| Cr I | 4 | ... | -0.42+-0.09 | 2.54+-0.09 | -3.10+-0.09 | -0.41+-0.09 | 2.54+-0.09 | Cr I |
| Mn I | 1 | ... | 0.24+-0.18 | 2.99+-0.18 | -2.44+-0.18 | 0.25+-0.18 | 2.99+-0.18 | Mn I |
| Fe I | 29 | ... | -0.01+-0.17 | 4.81+-0.17 | -2.69+-0.17 | -0.01+-0.17 | 4.81+-0.17 | Fe I |
| Fe II | 3 | ... | 0.09+-0.14 | 4.91+-0.14 | -2.59+-0.14 | 0.09+-0.14 | 4.91+-0.14 | Fe II |
| Ni I | 1 | ... | -0.29+-0.18 | 3.25+-0.18 | -2.97+-0.18 | -0.28+-0.18 | 3.25+-0.18 | Ni I |
| Sr II | 2 | ... | 0.38+-0.13 | 0.57+-0.13 | -2.30+-0.13 | 0.39+-0.13 | 0.57+-0.13 | Sr II |
| Ba II | 2 | ... | -0.21+-0.13 | -0.71+-0.13 | -2.89+-0.13 | -0.20+-0.13 | -0.71+-0.13 | Ba II |
| Right Ascension : 03 57 24.54 | Declination : +32 43 03.78 | 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 | 13.8 | N/A | 114.3 |