J1220+1637
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6376+-198 | log g : 3.79+-0.08 | vturb : 0.65+-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 |
| C | ... | <1.50 | <7.21 | <-1.22 | <1.48 | <7.21 | C | |
| Na I | 2 | ... | -0.39+-0.17 | 3.13+-0.17 | -3.11+-0.17 | -0.41+-0.17 | 3.13+-0.17 | Na I |
| Mg I | 2 | ... | -0.45+-0.13 | 4.43+-0.13 | -3.17+-0.13 | -0.47+-0.13 | 4.43+-0.13 | Mg I |
| Ca I | 1 | ... | -0.34+-0.18 | 3.28+-0.18 | -3.06+-0.18 | -0.36+-0.18 | 3.28+-0.18 | Ca I |
| Sc II | 1 | ... | -0.01+-0.20 | 0.42+-0.20 | -2.73+-0.20 | -0.03+-0.20 | 0.42+-0.20 | Sc II |
| Ti II | 6 | ... | 0.35+-0.14 | 2.58+-0.14 | -2.37+-0.14 | 0.33+-0.14 | 2.58+-0.14 | Ti II |
| Cr I | 1 | ... | 0.18+-0.19 | 3.10+-0.19 | -2.54+-0.19 | 0.16+-0.19 | 3.10+-0.19 | Cr I |
| Fe I | 14 | ... | 0.02+-0.17 | 4.80+-0.17 | -2.70+-0.17 | 0.02+-0.17 | 4.80+-0.17 | Fe I |
| Fe II | 2 | ... | -0.04+-0.34 | 4.74+-0.34 | -2.76+-0.34 | -0.04+-0.34 | 4.74+-0.34 | Fe II |
| Ni I | 1 | ... | 0.03+-0.19 | 3.53+-0.19 | -2.69+-0.19 | 0.01+-0.19 | 3.53+-0.19 | Ni I |
| Sr II | 1 | ... | 0.15+-0.19 | 0.30+-0.19 | -2.57+-0.19 | 0.13+-0.19 | 0.30+-0.19 | Sr II |
| Right Ascension : 12 20 46.05 | Declination : +16 37 05.47 | 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 | 23.3 | N/A | -38.9 |