J0815+3051
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6451+-136 | log g : 3.87+-0.07 | vturb : 0.94+-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 | ... | 2.22+-0.23 | 2.22+-0.23 | -1.04+-0.23 | 1.33+-0.23 | 2.22+-0.23 | Li I |
| Mg I | 2 | ... | -0.05+-0.16 | 5.19+-0.16 | -2.41+-0.16 | -0.04+-0.16 | 5.19+-0.16 | Mg I |
| Ca I | 4 | ... | 0.06+-0.15 | 4.04+-0.15 | -2.30+-0.15 | 0.07+-0.15 | 4.04+-0.15 | Ca I |
| Sc II | 2 | ... | -0.14+-0.16 | 0.65+-0.16 | -2.50+-0.16 | -0.13+-0.16 | 0.65+-0.16 | Sc II |
| Ti II | 9 | ... | 0.23+-0.12 | 2.82+-0.12 | -2.13+-0.12 | 0.24+-0.12 | 2.82+-0.12 | Ti II |
| Cr I | 4 | ... | -0.12+-0.12 | 3.16+-0.12 | -2.48+-0.12 | -0.11+-0.12 | 3.16+-0.12 | Cr I |
| Fe I | 33 | ... | -0.01+-0.21 | 5.13+-0.21 | -2.37+-0.21 | -0.01+-0.21 | 5.13+-0.21 | Fe I |
| Fe II | 3 | ... | -0.37+-0.22 | 4.77+-0.22 | -2.73+-0.22 | -0.37+-0.22 | 4.77+-0.22 | Fe II |
| Sr II | 2 | ... | 0.37+-0.25 | 0.88+-0.25 | -1.99+-0.25 | 0.38+-0.25 | 0.88+-0.25 | Sr II |
| Right Ascension : 08 15 56.35 | Declination : +30 51 56.60 | 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 | 20.6 | N/A | 158.3 |