HE0122-1616
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
| Teff : 5215+-100 | log g : 2.5+-0.25 | vturb : 1.8+-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 | ... | 0.21 | ... | -2.43 | 0.42 | 6.00 | CH |
| Na I | 2 | ... | -0.24+-0.03 | ... | -2.96+-0.03 | -0.11+-0.03 | 3.28+-0.03 | Na I |
| Mg I | 5 | ... | 0.28+-0.07 | ... | -2.58+-0.07 | 0.27+-0.07 | 5.02+-0.07 | Mg I |
| Ca I | 9 | ... | 0.22+-0.17 | ... | -2.56+-0.17 | 0.29+-0.17 | 3.78+-0.17 | Ca I |
| Ti I | 7 | ... | 0.06+-0.11 | ... | -2.70+-0.11 | 0.15+-0.11 | 2.25+-0.11 | Ti I |
| Ti II | 11 | ... | 0.01+-0.15 | ... | -2.75+-0.15 | 0.10+-0.15 | 2.20+-0.15 | Ti II |
| Cr I | 3 | ... | -0.5+-0.1 | ... | -3.27+-0.1 | -0.42+-0.1 | 2.37+-0.1 | Cr I |
| Mn I | 2 | ... | -1.23+-0.02 | ... | -4.07+-0.02 | -1.22+-0.02 | 1.36+-0.02 | Mn I |
| Fe I | N/A | -2.8+-0.19 | ... | ... | -2.85+-0.19 | ... | 4.65+-0.19 | Fe I |
| Fe II | 11 | -2.85+-0.14 | -0.05+-0.14 | ... | -2.90+-0.14 | -0.05+-0.14 | 4.60+-0.14 | Fe II |
| Co I | 4 | ... | 0.33+-0.21 | ... | -2.54+-0.21 | 0.31+-0.21 | 2.45+-0.21 | Co I |
| Ni I | 2 | ... | -0.33+-0.18 | ... | -3.10+-0.18 | -0.25+-0.18 | 3.12+-0.18 | Ni I |
| Zn I | 1 | ... | 0.08 | ... | -2.68 | 0.17 | 1.88 | Zn I |
| Sr II | 1 | ... | -0.42 | ... | -3.19 | -0.34 | -0.32 | Sr II |
| Ba II | 1 | ... | -1.07 | ... | -3.92 | -1.07 | -1.74 | Ba II |
| Vrad | 207.7 |
| Right Ascension : 01 25 10.80 | Declination : -16 00 54.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2005-09 | N/A | KECKHIRES | 36000 | 150 | 10800 | 207.7 |