J1327+0710
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6101+-118 | log g : 4.33+-0.04 | vturb : 1.07+-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 | ... | 1.92+-0.15 | 1.92+-0.15 | -1.34+-0.15 | 1.92+-0.15 | 1.92+-0.15 | Li I |
| C | 1 | ... | 1.65+-0.17 | 6.83+-0.17 | -1.60+-0.17 | 1.66+-0.17 | 6.83+-0.17 | C |
| Na I | 2 | ... | -0.48+-0.11 | 2.51+-0.11 | -3.73+-0.11 | -0.47+-0.11 | 2.51+-0.11 | Na I |
| Mg I | 4 | ... | 0.33+-0.18 | 4.68+-0.18 | -2.92+-0.18 | 0.34+-0.18 | 4.68+-0.18 | Mg I |
| Ca I | 1 | ... | 0.97+-0.14 | 4.06+-0.14 | -2.28+-0.14 | 0.98+-0.14 | 4.06+-0.14 | Ca I |
| Sc II | 1 | ... | 0.74+-0.14 | 0.64+-0.14 | -2.51+-0.14 | 0.75+-0.14 | 0.64+-0.14 | Sc II |
| Ti II | 3 | ... | 0.79+-0.23 | 2.49+-0.23 | -2.46+-0.23 | 0.80+-0.23 | 2.49+-0.23 | Ti II |
| Cr I | 4 | ... | -0.01+-0.24 | 2.38+-0.24 | -3.26+-0.24 | 0.00+-0.24 | 2.38+-0.24 | Cr I |
| Fe I | 12 | ... | -0.01+-0.13 | 4.24+-0.13 | -3.26+-0.13 | -0.01+-0.13 | 4.24+-0.13 | Fe I |
| Fe II | 2 | ... | -0.05+-0.40 | 4.20+-0.40 | -3.30+-0.40 | -0.05+-0.40 | 4.20+-0.40 | Fe II |
| Sr II | 2 | ... | 0.10+-0.10 | -0.28+-0.10 | -3.15+-0.10 | 0.11+-0.10 | -0.28+-0.10 | Sr II |
| Right Ascension : 13 27 29.06 | Declination : +07 10 51.97 | 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 | 33.2 | N/A | -18.6 |