J0409+2009
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 4317+-48 | log g : 0.62+-0.10 | vturb : 2.36+-0.09 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| C | ... | <-0.98 | <4.08 | <-4.35 | <-0.97 | <4.08 | C | |
| Mg I | 5 | ... | 0.98+-0.18 | 5.21+-0.18 | -2.39+-0.18 | 0.99+-0.18 | 5.21+-0.18 | Mg I |
| Si I | 1 | ... | 0.63+-0.11 | 4.77+-0.11 | -2.74+-0.11 | 0.64+-0.11 | 4.77+-0.11 | Si I |
| Ca I | 22 | ... | 0.88+-0.11 | 3.85+-0.11 | -2.49+-0.11 | 0.89+-0.11 | 3.85+-0.11 | Ca I |
| Sc II | 12 | ... | 0.44+-0.14 | 0.22+-0.14 | -2.93+-0.14 | 0.45+-0.14 | 0.22+-0.14 | Sc II |
| Ti II | 30 | ... | 0.54+-0.16 | 2.12+-0.16 | -2.83+-0.16 | 0.55+-0.16 | 2.12+-0.16 | Ti II |
| V I | 1 | ... | 0.03+-0.11 | 0.59+-0.11 | -3.34+-0.11 | 0.04+-0.11 | 0.59+-0.11 | V I |
| Cr I | 8 | ... | -0.26+-0.15 | 2.01+-0.15 | -3.63+-0.15 | -0.25+-0.15 | 2.01+-0.15 | Cr I |
| Fe I | 108 | ... | -0.01+-0.11 | 4.12+-0.11 | -3.38+-0.11 | -0.01+-0.11 | 4.12+-0.11 | Fe I |
| Fe II | 14 | ... | 0.28+-0.20 | 4.41+-0.20 | -3.09+-0.20 | 0.28+-0.20 | 4.41+-0.20 | Fe II |
| Co I | 2 | ... | -0.38+-0.08 | 1.24+-0.08 | -3.75+-0.08 | -0.37+-0.08 | 1.24+-0.08 | Co I |
| Ni I | 3 | ... | 0.28+-0.13 | 3.13+-0.13 | -3.09+-0.13 | 0.29+-0.13 | 3.13+-0.13 | Ni I |
| Right Ascension : 04 09 09.71 | Declination : +20 09 52.91 | 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 | 26.8 | N/A | 26.5 |