J1544+0901
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6583+-146 | log g : 3.93+-0.07 | vturb : 1.38+-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 | ... | <1.80 | <7.42 | <-1.01 | <1.79 | <7.42 | C | |
| Na I | 1 | ... | -0.50+-0.15 | 2.93+-0.15 | -3.31+-0.15 | -0.51+-0.15 | 2.93+-0.15 | Na I |
| Mg I | 3 | ... | 0.22+-0.10 | 5.01+-0.10 | -2.59+-0.10 | 0.21+-0.10 | 5.01+-0.10 | Mg I |
| Ca I | 3 | ... | 0.22+-0.25 | 3.75+-0.25 | -2.59+-0.25 | 0.21+-0.25 | 3.75+-0.25 | Ca I |
| Sc II | 1 | ... | 0.14+-0.14 | 0.48+-0.14 | -2.67+-0.14 | 0.13+-0.14 | 0.48+-0.14 | Sc II |
| Ti II | 5 | ... | 0.26+-0.14 | 2.40+-0.14 | -2.55+-0.14 | 0.25+-0.14 | 2.40+-0.14 | Ti II |
| Cr I | 1 | ... | -0.05+-0.14 | 2.78+-0.14 | -2.86+-0.14 | -0.06+-0.14 | 2.78+-0.14 | Cr I |
| Fe I | 17 | ... | 0.01+-0.12 | 4.70+-0.12 | -2.80+-0.12 | 0.01+-0.12 | 4.70+-0.12 | Fe I |
| Fe II | 2 | ... | -0.15+-0.17 | 4.54+-0.17 | -2.96+-0.17 | -0.15+-0.17 | 4.54+-0.17 | Fe II |
| Sr II | 2 | ... | -0.23+-0.10 | -0.17+-0.10 | -3.04+-0.10 | -0.24+-0.10 | -0.17+-0.10 | Sr II |
| Right Ascension : 15 44 26.36 | Declination : +09 01 05.56 | 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 | 28.2 | N/A | -109.1 |