G166-45B
Examination of the Mass-dependent Li Depletion Hypothesis by the Li Abundances of the Very Metal-poor Double-lined Spectroscopic Binary G166-45
| Teff : 5830+-170 | log g : 4.6+-0.3 | vturb : 1.0+-0.2 |
| 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+-0.03 | -1.15+-0.03 | 1.25+-0.03 | 2.11+-0.03 | Li I |
| Na I | 2 | ... | -0.08+-0.09 | 3.76+-0.09 | -2.48+-0.09 | -0.08+-0.09 | 3.76+-0.09 | Na I |
| Mg I | 3 | ... | 0.11+-0.12 | 5.31+-0.12 | -2.29+-0.12 | 0.11+-0.12 | 5.31+-0.12 | Mg I |
| Ca I | 8 | ... | 0.26+-0.08 | 4.20+-0.08 | -2.14+-0.08 | 0.26+-0.08 | 4.20+-0.08 | Ca I |
| Ti II | 3 | ... | 0.46+-0.13 | 3.01+-0.13 | -1.94+-0.13 | 0.46+-0.13 | 3.01+-0.13 | Ti II |
| Cr I | 3 | ... | -0.10+-0.10 | 3.14+-0.10 | -2.50+-0.10 | -0.10+-0.10 | 3.14+-0.10 | Cr I |
| Fe I | 39 | -2.40+-0.11 | ... | 5.10+-0.11 | -2.40+-0.11 | ... | 5.10+-0.11 | Fe I |
| Fe II | 2 | -2.20+-0.15 | ... | 5.30+-0.15 | -2.20+-0.15 | ... | 5.30+-0.15 | Fe II |
| Ni I | 2 | ... | 0.35+-0.13 | 4.17+-0.13 | -2.05+-0.13 | 0.35+-0.13 | 4.17+-0.13 | Ni I |
| Binarity | Positive |
| Right Ascension : 14 49 02.36 | Declination : +25 42 09.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2011-07-22 | N/A | SUBARUHDS | 110000 | 350 | 3600 | N/A |