J0025+2305
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6308+-144 | log g : 3.93+-0.04 | vturb : 1.99+-0.17 |
| 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 | ... | 2.30+-0.10 | 2.30+-0.10 | -0.96+-0.10 | 1.85+-0.10 | 2.30+-0.10 | Li I |
| C | ... | <1.27 | <6.89 | <-1.54 | <1.27 | <6.89 | C | |
| Na I | 2 | ... | -0.78+-0.09 | 2.65+-0.09 | -3.59+-0.09 | -0.78+-0.09 | 2.65+-0.09 | Na I |
| Mg I | 2 | ... | -0.16+-0.08 | 4.63+-0.08 | -2.97+-0.08 | -0.16+-0.08 | 4.63+-0.08 | Mg I |
| Ca I | 7 | ... | 0.36+-0.16 | 3.89+-0.16 | -2.45+-0.16 | 0.36+-0.16 | 3.89+-0.16 | Ca I |
| Sc II | 3 | ... | 0.11+-0.10 | 0.45+-0.10 | -2.70+-0.10 | 0.11+-0.10 | 0.45+-0.10 | Sc II |
| Ti II | 12 | ... | 0.33+-0.12 | 2.47+-0.12 | -2.48+-0.12 | 0.33+-0.12 | 2.47+-0.12 | Ti II |
| Cr I | 5 | ... | -0.07+-0.11 | 2.76+-0.11 | -2.88+-0.11 | -0.07+-0.11 | 2.76+-0.11 | Cr I |
| Fe I | 34 | ... | 0.00+-0.10 | 4.69+-0.10 | -2.81+-0.10 | 0.00+-0.10 | 4.69+-0.10 | Fe I |
| Fe II | 8 | ... | 0.15+-0.17 | 4.84+-0.17 | -2.66+-0.17 | 0.15+-0.17 | 4.84+-0.17 | Fe II |
| Sr II | 2 | ... | -0.24+-0.08 | -0.18+-0.08 | -3.05+-0.08 | -0.24+-0.08 | -0.18+-0.08 | Sr II |
| Right Ascension : 00 25 43.77 | Declination : +23 05 36.82 | 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 | 48.3 | N/A | -229.6 |