J0749+4629
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6164+-124 | log g : 3.95+-0.04 | vturb : 1.57+-0.17 |
| 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 | ... | 2.25+-0.15 | 2.25+-0.15 | -1.01+-0.15 | 1.40+-0.15 | 2.25+-0.15 | Li I |
| C | ... | <0.70 | <6.72 | <-1.71 | <0.70 | <6.72 | C | |
| Na I | 2 | ... | -0.02+-0.11 | 3.81+-0.11 | -2.43+-0.11 | -0.02+-0.11 | 3.81+-0.11 | Na I |
| Mg I | 4 | ... | 0.31+-0.13 | 5.50+-0.13 | -2.10+-0.13 | 0.31+-0.13 | 5.50+-0.13 | Mg I |
| Ca I | 6 | ... | 0.37+-0.15 | 4.30+-0.15 | -2.04+-0.15 | 0.37+-0.15 | 4.30+-0.15 | Ca I |
| Sc II | 2 | ... | 0.34+-0.14 | 1.08+-0.14 | -2.07+-0.14 | 0.34+-0.14 | 1.08+-0.14 | Sc II |
| Ti II | 14 | ... | 0.47+-0.15 | 3.01+-0.15 | -1.94+-0.15 | 0.47+-0.15 | 3.01+-0.15 | Ti II |
| Cr I | 5 | ... | -0.19+-0.14 | 3.04+-0.14 | -2.60+-0.14 | -0.19+-0.14 | 3.04+-0.14 | Cr I |
| Fe I | 50 | ... | 0.00+-0.15 | 5.09+-0.15 | -2.41+-0.15 | 0.00+-0.15 | 5.09+-0.15 | Fe I |
| Fe II | 6 | ... | 0.05+-0.18 | 5.14+-0.18 | -2.36+-0.18 | 0.05+-0.18 | 5.14+-0.18 | Fe II |
| Sr II | 2 | ... | -0.47+-0.11 | -0.01+-0.11 | -2.88+-0.11 | -0.47+-0.11 | -0.01+-0.11 | Sr II |
| Right Ascension : 07 49 25.16 | Declination : +46 29 17.30 | 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 | 24.9 | N/A | 116.0 |