J1446+3712
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6242+-68 | log g : 4.53+-0.02 | vturb : 2.90+-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 | ... | 2.11+-0.13 | 2.11+-0.13 | -1.15+-0.13 | 1.87+-0.13 | 2.11+-0.13 | Li I |
| C | ... | <1.40 | <6.80 | <-1.63 | <1.39 | <6.80 | C | |
| Na I | 2 | ... | -0.29+-0.09 | 2.92+-0.09 | -3.32+-0.09 | -0.30+-0.09 | 2.92+-0.09 | Na I |
| Mg I | 2 | ... | 0.00+-0.10 | 4.57+-0.10 | -3.03+-0.10 | -0.01+-0.10 | 4.57+-0.10 | Mg I |
| Ca I | 3 | ... | 0.40+-0.13 | 3.71+-0.13 | -2.63+-0.13 | 0.39+-0.13 | 3.71+-0.13 | Ca I |
| Sc II | 1 | ... | 0.27+-0.13 | 0.39+-0.13 | -2.76+-0.13 | 0.26+-0.13 | 0.39+-0.13 | Sc II |
| Ti II | 8 | ... | 0.46+-0.15 | 2.38+-0.15 | -2.57+-0.15 | 0.45+-0.15 | 2.38+-0.15 | Ti II |
| Cr I | 5 | ... | -0.14+-0.13 | 2.47+-0.13 | -3.17+-0.13 | -0.15+-0.13 | 2.47+-0.13 | Cr I |
| Fe I | 21 | ... | 0.01+-0.13 | 4.48+-0.13 | -3.02+-0.13 | 0.01+-0.13 | 4.48+-0.13 | Fe I |
| Fe II | 2 | ... | -0.15+-0.10 | 4.32+-0.10 | -3.18+-0.10 | -0.15+-0.10 | 4.32+-0.10 | Fe II |
| Sr II | 2 | ... | -0.40+-0.09 | -0.56+-0.09 | -3.43+-0.09 | -0.41+-0.09 | -0.56+-0.09 | Sr II |
| Right Ascension : 14 46 37.23 | Declination : +37 12 27.99 | 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 | 33.4 | N/A | -175.0 |