J1650+0438
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 5112+-50 | log g : 2.36+-0.30 | vturb : 3.30+-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 |
| C | 1 | ... | 2.00+-0.29 | 6.84+-0.29 | -1.59+-0.29 | 2.01+-0.29 | 6.84+-0.29 | C |
| Na I | 2 | ... | -0.20+-0.18 | 2.45+-0.18 | -3.79+-0.18 | -0.19+-0.18 | 2.45+-0.18 | Na I |
| Mg I | 3 | ... | 0.18+-0.26 | 4.19+-0.26 | -3.41+-0.26 | 0.19+-0.26 | 4.19+-0.26 | Mg I |
| Ca I | 2 | ... | 0.36+-0.21 | 3.11+-0.21 | -3.23+-0.21 | 0.37+-0.21 | 3.11+-0.21 | Ca I |
| Sc II | 2 | ... | 0.33+-0.21 | -0.11+-0.21 | -3.26+-0.21 | 0.34+-0.21 | -0.11+-0.21 | Sc II |
| Ti II | 7 | ... | 0.29+-0.17 | 1.65+-0.17 | -3.30+-0.17 | 0.30+-0.17 | 1.65+-0.17 | Ti II |
| Cr I | 1 | ... | -0.20+-0.26 | 1.85+-0.26 | -3.79+-0.26 | -0.19+-0.26 | 1.85+-0.26 | Cr I |
| Fe I | 19 | ... | -0.01+-0.25 | 3.90+-0.25 | -3.60+-0.25 | -0.01+-0.25 | 3.90+-0.25 | Fe I |
| Fe II | 4 | ... | 0.07+-0.43 | 3.98+-0.43 | -3.52+-0.43 | 0.07+-0.43 | 3.98+-0.43 | Fe II |
| Sr II | 2 | ... | -0.29+-0.27 | -1.01+-0.27 | -3.88+-0.27 | -0.28+-0.27 | -1.01+-0.27 | Sr II |
| Right Ascension : 16 50 44.46 | Declination : +04 38 36.17 | 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 | 18.0 | N/A | 5.8 |
| N/A | N/A | SUBARUHDS | 36000 | 16.3 | N/A | -429.8 |