J0232+4115
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 5754+-114 | log g : 2.42+-0.15 | vturb : 2.68+-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 | ... | <1.43 | <6.66 | <-1.77 | <1.41 | <6.66 | C | |
| Na I | 2 | ... | -0.02+-0.10 | 3.02+-0.10 | -3.22+-0.10 | -0.04+-0.10 | 3.02+-0.10 | Na I |
| Mg I | 3 | ... | 0.72+-0.35 | 5.12+-0.35 | -2.48+-0.35 | 0.70+-0.35 | 5.12+-0.35 | Mg I |
| Ca I | 2 | ... | 0.56+-0.15 | 3.70+-0.15 | -2.64+-0.15 | 0.54+-0.15 | 3.70+-0.15 | Ca I |
| Sc II | 4 | ... | 0.31+-0.18 | 0.26+-0.18 | -2.89+-0.18 | 0.29+-0.18 | 0.26+-0.18 | Sc II |
| Ti II | 10 | ... | 0.62+-0.16 | 2.37+-0.16 | -2.58+-0.16 | 0.60+-0.16 | 2.37+-0.16 | Ti II |
| Cr I | 1 | ... | -0.38+-0.13 | 2.06+-0.13 | -3.58+-0.13 | -0.40+-0.13 | 2.06+-0.13 | Cr I |
| Fe I | 14 | ... | 0.02+-0.12 | 4.32+-0.12 | -3.18+-0.12 | 0.02+-0.12 | 4.32+-0.12 | Fe I |
| Fe II | 3 | ... | 0.19+-0.12 | 4.49+-0.12 | -3.01+-0.12 | 0.19+-0.12 | 4.49+-0.12 | Fe II |
| Sr II | 2 | ... | 1.27+-0.17 | 0.94+-0.17 | -1.93+-0.17 | 1.25+-0.17 | 0.94+-0.17 | Sr II |
| Ba II | 2 | ... | 0.07+-0.11 | -0.95+-0.11 | -3.13+-0.11 | 0.05+-0.11 | -0.95+-0.11 | Ba II |
| Right Ascension : 02 32 18.79 | Declination : +41 15 44.70 | 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 | 21.5 | N/A | -454.7 |
| N/A | N/A | SUBARUHDS | 36000 | 29.5 | N/A | -454.0 |