J0054+2649
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6320+-134 | log g : 4.07+-0.04 | vturb : 1.45+-0.23 |
| 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 | ... | 1.95+-0.17 | 1.95+-0.17 | -1.31+-0.17 | 1.91+-0.17 | 1.95+-0.17 | Li I |
| C | ... | <1.40 | <6.61 | <-1.82 | <1.40 | <6.61 | C | |
| Na I | 1 | ... | -0.07+-0.12 | 2.95+-0.12 | -3.29+-0.12 | -0.07+-0.12 | 2.95+-0.12 | Na I |
| Mg I | 4 | ... | 0.48+-0.11 | 4.86+-0.11 | -2.74+-0.11 | 0.48+-0.11 | 4.86+-0.11 | Mg I |
| Ca I | 2 | ... | 0.56+-0.10 | 3.68+-0.10 | -2.66+-0.10 | 0.56+-0.10 | 3.68+-0.10 | Ca I |
| Sc II | 1 | ... | 0.31+-0.13 | 0.24+-0.13 | -2.91+-0.13 | 0.31+-0.13 | 0.24+-0.13 | Sc II |
| Ti II | 8 | ... | 0.49+-0.14 | 2.22+-0.14 | -2.73+-0.14 | 0.49+-0.14 | 2.22+-0.14 | Ti II |
| Cr I | 2 | ... | -0.25+-0.21 | 2.17+-0.21 | -3.47+-0.21 | -0.25+-0.21 | 2.17+-0.21 | Cr I |
| Fe I | 18 | ... | 0.00+-0.12 | 4.28+-0.12 | -3.22+-0.12 | 0.00+-0.12 | 4.28+-0.12 | Fe I |
| Fe II | 2 | ... | -0.06+-0.11 | 4.22+-0.11 | -3.28+-0.11 | -0.06+-0.11 | 4.22+-0.11 | Fe II |
| Sr II | 2 | ... | -0.09+-0.10 | -0.44+-0.10 | -3.31+-0.10 | -0.09+-0.10 | -0.44+-0.10 | Sr II |
| Right Ascension : 00 54 03.15 | Declination : +26 49 09.74 | 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 | 55.8 | N/A | -307.5 |