J1705+0855
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6306+-121 | log g : 4.32+-0.03 | vturb : 1.75+-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 | ... | 2.06+-0.20 | 2.06+-0.20 | -1.20+-0.20 | 1.75+-0.20 | 2.06+-0.20 | Li I |
| C | ... | <1.30 | <6.78 | <-1.65 | <1.30 | <6.78 | C | |
| Na I | 2 | ... | -0.41+-0.14 | 2.88+-0.14 | -3.36+-0.14 | -0.41+-0.14 | 2.88+-0.14 | Na I |
| Mg I | 5 | ... | 0.27+-0.14 | 4.92+-0.14 | -2.68+-0.14 | 0.27+-0.14 | 4.92+-0.14 | Mg I |
| Ca I | 7 | ... | 0.27+-0.15 | 3.66+-0.15 | -2.68+-0.15 | 0.27+-0.15 | 3.66+-0.15 | Ca I |
| Sc II | 1 | ... | 0.43+-0.20 | 0.63+-0.20 | -2.52+-0.20 | 0.43+-0.20 | 0.63+-0.20 | Sc II |
| Ti II | 9 | ... | 0.38+-0.12 | 2.38+-0.12 | -2.57+-0.12 | 0.38+-0.12 | 2.38+-0.12 | Ti II |
| Cr I | 5 | ... | -0.25+-0.11 | 2.44+-0.11 | -3.20+-0.11 | -0.25+-0.11 | 2.44+-0.11 | Cr I |
| Fe I | 37 | ... | 0.00+-0.20 | 4.55+-0.20 | -2.95+-0.20 | 0.00+-0.20 | 4.55+-0.20 | Fe I |
| Fe II | 3 | ... | -0.09+-0.16 | 4.46+-0.16 | -3.04+-0.16 | -0.09+-0.16 | 4.46+-0.16 | Fe II |
| Sr II | 2 | ... | -0.31+-0.14 | -0.39+-0.14 | -3.26+-0.14 | -0.31+-0.14 | -0.39+-0.14 | Sr II |
| Right Ascension : 17 05 29.80 | Declination : +08 55 59.17 | 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 | 48.4 | N/A | 44.0 |