J0632+2105
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 5706+-114 | log g : 3.81+-0.04 | vturb : 1.29+-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 | ... | 1.81+-0.23 | 1.81+-0.23 | -1.45+-0.23 | 1.97+-0.23 | 1.81+-0.23 | Li I |
| C | ... | <0.78 | <5.80 | <-2.63 | <0.79 | <5.80 | C | |
| Na I | 2 | ... | -0.22+-0.16 | 2.61+-0.16 | -3.63+-0.16 | -0.21+-0.16 | 2.61+-0.16 | Na I |
| Mg I | 4 | ... | 0.38+-0.14 | 4.57+-0.14 | -3.03+-0.14 | 0.39+-0.14 | 4.57+-0.14 | Mg I |
| Ca I | 3 | ... | 0.29+-0.25 | 3.22+-0.25 | -3.12+-0.25 | 0.30+-0.25 | 3.22+-0.25 | Ca I |
| Sc II | 2 | ... | 0.42+-0.16 | 0.16+-0.16 | -2.99+-0.16 | 0.43+-0.16 | 0.16+-0.16 | Sc II |
| Ti II | 13 | ... | 0.70+-0.12 | 2.24+-0.12 | -2.71+-0.12 | 0.71+-0.12 | 2.24+-0.12 | Ti II |
| Cr I | 5 | ... | -0.27+-0.12 | 1.96+-0.12 | -3.68+-0.12 | -0.26+-0.12 | 1.96+-0.12 | Cr I |
| Fe I | 26 | ... | -0.01+-0.22 | 4.08+-0.22 | -3.42+-0.22 | -0.01+-0.22 | 4.08+-0.22 | Fe I |
| Fe II | 3 | ... | 0.31+-0.12 | 4.40+-0.12 | -3.10+-0.12 | 0.31+-0.12 | 4.40+-0.12 | Fe II |
| Sr II | 2 | ... | 0.72+-0.20 | 0.18+-0.20 | -2.69+-0.20 | 0.73+-0.20 | 0.18+-0.20 | Sr II |
| Ba II | 2 | ... | 0.47+-0.16 | -0.76+-0.16 | -2.94+-0.16 | 0.48+-0.16 | -0.76+-0.16 | Ba II |
| Right Ascension : 06 32 38.10 | Declination : +21 05 31.52 | 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 | 26.9 | N/A | -117.6 |