J1421+2401
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6590+-104 | log g : 4.25+-0.03 | vturb : 1.91+-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 | ... | 2.42+-0.14 | 2.42+-0.14 | -0.84+-0.14 | 1.84+-0.14 | 2.42+-0.14 | Li I |
| C | ... | <1.50 | <7.25 | <-1.18 | <1.50 | <7.25 | C | |
| Na I | 2 | ... | -0.41+-0.10 | 3.15+-0.10 | -3.09+-0.10 | -0.41+-0.10 | 3.15+-0.10 | Na I |
| Mg I | 3 | ... | 0.24+-0.10 | 5.16+-0.10 | -2.44+-0.10 | 0.24+-0.10 | 5.16+-0.10 | Mg I |
| Ca I | 7 | ... | 0.48+-0.13 | 4.14+-0.13 | -2.20+-0.13 | 0.48+-0.13 | 4.14+-0.13 | Ca I |
| Sc II | 3 | ... | 0.71+-0.23 | 1.18+-0.23 | -1.97+-0.23 | 0.71+-0.23 | 1.18+-0.23 | Sc II |
| Ti II | 14 | ... | 0.50+-0.13 | 2.77+-0.13 | -2.18+-0.13 | 0.50+-0.13 | 2.77+-0.13 | Ti II |
| Cr I | 4 | ... | -0.15+-0.17 | 2.81+-0.17 | -2.83+-0.17 | -0.15+-0.17 | 2.81+-0.17 | Cr I |
| Fe I | 31 | ... | 0.00+-0.14 | 4.82+-0.14 | -2.68+-0.14 | 0.00+-0.14 | 4.82+-0.14 | Fe I |
| Fe II | 3 | ... | 0.11+-0.16 | 4.93+-0.16 | -2.57+-0.16 | 0.11+-0.16 | 4.93+-0.16 | Fe II |
| Sr II | 2 | ... | 0.10+-0.19 | 0.29+-0.19 | -2.58+-0.19 | 0.10+-0.19 | 0.29+-0.19 | Sr II |
| Right Ascension : 14 21 50.54 | Declination : +24 01 59.08 | 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 | 39.0 | N/A | -47.7 |