J0037+2935
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6019+-93 | log g : 4.37+-0.03 | vturb : 1.15+-0.27 |
| 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 | ... | 1.98+-0.18 | 1.98+-0.18 | -1.28+-0.18 | 1.62+-0.18 | 1.98+-0.18 | Li I |
| C | ... | <1.10 | <6.64 | <-1.79 | <1.11 | <6.64 | C | |
| Na I | 2 | ... | -0.57+-0.14 | 2.78+-0.14 | -3.46+-0.14 | -0.56+-0.14 | 2.78+-0.14 | Na I |
| Mg I | 3 | ... | 0.36+-0.10 | 5.07+-0.10 | -2.53+-0.10 | 0.37+-0.10 | 5.07+-0.10 | Mg I |
| Ca I | 3 | ... | 0.46+-0.23 | 3.91+-0.23 | -2.43+-0.23 | 0.47+-0.23 | 3.91+-0.23 | Ca I |
| Sc II | 1 | ... | 0.22+-0.18 | 0.48+-0.18 | -2.67+-0.18 | 0.23+-0.18 | 0.48+-0.18 | Sc II |
| Ti II | 10 | ... | 0.60+-0.22 | 2.66+-0.22 | -2.29+-0.22 | 0.61+-0.22 | 2.66+-0.22 | Ti II |
| Cr I | 3 | ... | -0.27+-0.11 | 2.48+-0.11 | -3.16+-0.11 | -0.26+-0.11 | 2.48+-0.11 | Cr I |
| Fe I | 37 | ... | -0.01+-0.18 | 4.60+-0.18 | -2.90+-0.18 | -0.01+-0.18 | 4.60+-0.18 | Fe I |
| Fe II | 3 | ... | -0.02+-0.17 | 4.59+-0.17 | -2.91+-0.17 | -0.02+-0.17 | 4.59+-0.17 | Fe II |
| Sr II | 2 | ... | 0.16+-0.15 | 0.14+-0.15 | -2.73+-0.15 | 0.17+-0.15 | 0.14+-0.15 | Sr II |
| Ba II | 1 | ... | 0.17+-0.18 | -0.54+-0.18 | -2.72+-0.18 | 0.18+-0.18 | -0.54+-0.18 | Ba II |
| Right Ascension : 00 37 07.81 | Declination : +29 35 06.19 | 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 | 19.1 | N/A | -31.9 |