HE1320+0139
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
| Teff : 5200+-100 | log g : 2.6+-0.25 | vturb : 1.4+-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 | ... | 0.35 | ... | -2.87 | 0.56 | 5.56 | CH |
| Na I | 2 | ... | -0.33+-0.01 | ... | -3.63+-0.01 | -0.20+-0.01 | 2.61+-0.01 | Na I |
| Mg I | 3 | ... | 0.01+-0.08 | ... | -3.43+-0.08 | -0.00+-0.08 | 4.17+-0.08 | Mg I |
| Al I | 1 | ... | -0.5 | ... | -3.86 | -0.43 | 2.59 | Al I |
| Si I | 1 | ... | 0.05 | ... | -3.29 | 0.14 | 4.22 | Si I |
| Ca I | 3 | ... | -0.19+-0.13 | ... | -3.55+-0.13 | -0.12+-0.13 | 2.79+-0.13 | Ca I |
| Sc II | 2 | ... | -0.01+-0.03 | ... | -3.44+-0.03 | -0.01+-0.03 | -0.29+-0.03 | Sc II |
| Ti II | 8 | ... | 0.03+-0.07 | ... | -3.31+-0.07 | 0.12+-0.07 | 1.64+-0.07 | Ti II |
| Cr I | 4 | ... | -0.52+-0.11 | ... | -3.87+-0.11 | -0.44+-0.11 | 1.77+-0.11 | Cr I |
| Mn I | 2 | ... | -0.62+-0.02 | ... | -4.04+-0.02 | -0.61+-0.02 | 1.39+-0.02 | Mn I |
| Fe I | N/A | -3.38+-0.16 | ... | ... | -3.43+-0.16 | ... | 4.07+-0.16 | Fe I |
| Fe II | 5 | -3.32+-0.08 | 0.06+-0.08 | ... | -3.37+-0.08 | 0.06+-0.08 | 4.13+-0.08 | Fe II |
| Co I | 1 | ... | 0.41 | ... | -3.04 | 0.39 | 1.95 | Co I |
| Ni I | 1 | ... | 0.49 | ... | -2.86 | 0.57 | 3.36 | Ni I |
| Sr II | 2 | ... | -1.02+-0.04 | ... | -4.37+-0.04 | -0.94+-0.04 | -1.50+-0.04 | Sr II |
| Ba II | 1 | ... | <-1.32 | ... | <-4.75 | <-1.32 | <-2.57 | Ba II |
| Vrad | 64.8 |
| Right Ascension : 13 22 50.60 | Declination : +01 23 42.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2004-05 | N/A | KECKHIRES | 36000 | 65 | 8400 | 64.8 |