J1028+2625
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6065+-86 | log g : 4.54+-0.04 | vturb : 1.20+-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 | ... | 2.16+-0.21 | 2.16+-0.21 | -1.10+-0.21 | 1.83+-0.21 | 2.16+-0.21 | Li I |
| C | ... | <1.05 | <6.57 | <-1.86 | <1.07 | <6.57 | C | |
| Na I | 2 | ... | -0.38+-0.14 | 2.95+-0.14 | -3.29+-0.14 | -0.36+-0.14 | 2.95+-0.14 | Na I |
| Mg I | 2 | ... | 0.26+-0.14 | 4.95+-0.14 | -2.65+-0.14 | 0.28+-0.14 | 4.95+-0.14 | Mg I |
| Ca I | 1 | ... | 0.22+-0.20 | 3.65+-0.20 | -2.69+-0.20 | 0.24+-0.20 | 3.65+-0.20 | Ca I |
| Ti II | 7 | ... | 0.49+-0.12 | 2.53+-0.12 | -2.42+-0.12 | 0.51+-0.12 | 2.53+-0.12 | Ti II |
| Cr I | 2 | ... | -0.01+-0.14 | 2.72+-0.14 | -2.92+-0.14 | 0.01+-0.14 | 2.72+-0.14 | Cr I |
| Fe I | 30 | ... | -0.02+-0.19 | 4.57+-0.19 | -2.93+-0.19 | -0.02+-0.19 | 4.57+-0.19 | Fe I |
| Fe II | 2 | ... | -0.18+-0.19 | 4.41+-0.19 | -3.09+-0.19 | -0.18+-0.19 | 4.41+-0.19 | Fe II |
| Sr II | 2 | ... | 0.07+-0.15 | 0.03+-0.15 | -2.84+-0.15 | 0.09+-0.15 | 0.03+-0.15 | Sr II |
| Right Ascension : 10 28 31.65 | Declination : +26 25 05.78 | 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 | 19.6 | N/A | -105.8 |