Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
| Teff : 5875 | log g : 4.31+-0.13 | vturb : 1.3 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Na I | 6 | ... | 0.13 | ... | -0.19 | 0.21 | 6.05 | Na I |
| Mg I | 7 | ... | 0.09 | ... | -0.34 | 0.06 | 7.26 | Mg I |
| Al I | 6 | ... | -0.02 | ... | -0.41 | -0.01 | 6.04 | Al I |
| Fe | N/A | -0.41 | ... | ... | -0.40 | ... | 7.10 | Fe |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| N/A | FOCES | 40000 | 200 | 5400 | N/A |
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -044637.4 | Right Ascension : 115903.02 |