HE0251-3216
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
| Teff : 5750+-100 | log g : 3.7+-0.25 | vturb : 1.6+-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 |
| CH | N/A | ... | 2.32 | ... | -0.67 | 2.53 | 7.76 | CH |
| Na I | 2 | ... | 0.84+-0.12 | ... | -2.23+-0.12 | 0.97+-0.12 | 4.01+-0.12 | Na I |
| Mg I | 4 | ... | 0.62+-0.07 | ... | -2.59+-0.07 | 0.61+-0.07 | 5.01+-0.07 | Mg I |
| Al I | 1 | ... | -0.02 | ... | -3.15 | 0.05 | 3.30 | Al I |
| Si I | 1 | ... | -0.69 | ... | -3.80 | -0.60 | 3.71 | Si I |
| Ca I | 3 | ... | 0.34+-0.21 | ... | -2.79+-0.21 | 0.41+-0.21 | 3.55+-0.21 | Ca I |
| Ti I | 1 | ... | 0.66 | ... | -2.45 | 0.75 | 2.50 | Ti I |
| Ti II | 7 | ... | 0.31+-0.2 | ... | -2.80+-0.2 | 0.40+-0.2 | 2.15+-0.2 | Ti II |
| Cr I | 2 | ... | -0.13+-0.08 | ... | -3.25+-0.08 | -0.05+-0.08 | 2.39+-0.08 | Cr I |
| Mn I | 2 | ... | -0.51+-0.04 | ... | -3.70+-0.04 | -0.50+-0.04 | 1.73+-0.04 | Mn I |
| Fe I | N/A | -3.15+-0.13 | ... | ... | -3.20+-0.13 | ... | 4.30+-0.13 | Fe I |
| Fe II | 2 | -3.24+-0.04 | -0.09+-0.04 | ... | -3.29+-0.04 | -0.09+-0.04 | 4.21+-0.04 | Fe II |
| Zn I | 1 | ... | 1.04 | ... | -2.07 | 1.13 | 2.49 | Zn I |
| Y II | 1 | ... | 1.33 | ... | -1.79 | 1.41 | 0.42 | Y II |
| Ba II | 4 | ... | 1.28+-0.11 | ... | -1.92+-0.11 | 1.28+-0.11 | 0.26+-0.11 | Ba II |
| Vrad | 94.9 |
| Right Ascension : 02 53 05.30 | Declination : -32 04 21.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2010-10 | N/A | KECKHIRES | 36000 | 90 | 1200 | 94.9 |