HE2155-3750

Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
| Teff : 5000+-100 | log g : 2.3+-0.25 | vturb : 1.7+-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 | ... | 1.7 | ... | -0.73 | 1.91 | 7.70 | CH |
| Na I | 2 | ... | 0.31+-0.15 | ... | -2.20+-0.15 | 0.44+-0.15 | 4.04+-0.15 | Na I |
| Mg I | 2 | ... | 0.55+-0.04 | ... | -2.10+-0.04 | 0.54+-0.04 | 5.50+-0.04 | Mg I |
| Si I | 2 | ... | 1.7+-0.3 | ... | -0.85+-0.3 | 1.79+-0.3 | 6.66+-0.3 | Si I |
| K I | 1 | ... | 1.09 | ... | -1.41 | 1.23 | 3.62 | K I |
| Ca I | 4 | ... | 0.69+-0.21 | ... | -1.88+-0.21 | 0.76+-0.21 | 4.46+-0.21 | Ca I |
| Sc II | 1 | ... | 0.53 | ... | -2.11 | 0.53 | 1.04 | Sc II |
| Ti I | 3 | ... | 0.73+-0.14 | ... | -1.82+-0.14 | 0.82+-0.14 | 3.13+-0.14 | Ti I |
| Ti II | 5 | ... | 0.82+-0.29 | ... | -1.73+-0.29 | 0.91+-0.29 | 3.22+-0.29 | Ti II |
| Cr I | 1 | ... | -0.38 | ... | -2.94 | -0.30 | 2.70 | Cr I |
| Fe I | N/A | -2.59+-0.2 | ... | ... | -2.64+-0.2 | ... | 4.86+-0.2 | Fe I |
| Fe II | 3 | -2.57+-0.3 | 0.02+-0.3 | ... | -2.62+-0.3 | 0.02+-0.3 | 4.88+-0.3 | Fe II |
| Y II | 5 | ... | 0.78+-0.15 | ... | -1.78+-0.15 | 0.86+-0.15 | 0.43+-0.15 | Y II |
| Ba II | 3 | ... | 1.92+-0.16 | ... | -0.72+-0.16 | 1.92+-0.16 | 1.46+-0.16 | Ba II |
| La II | 5 | ... | 1.65+-0.17 | ... | -0.90+-0.17 | 1.74+-0.17 | 0.20+-0.17 | La II |
| Ce II | 2 | ... | 1.74+-0.02 | ... | -0.88+-0.02 | 1.76+-0.02 | 0.70+-0.02 | Ce II |
| Nd II | 4 | ... | 1.89+-0.18 | ... | -0.62+-0.18 | 2.02+-0.18 | 0.80+-0.18 | Nd II |
| Eu II | 1 | ... | <1.65 | ... | <-0.95 | <1.69 | <-0.43 | Eu II |
| Vrad | 62.2 |
| Right Ascension : 21 58 09.80 | Declination : -37 36 20.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2004-10 | N/A | MIKELCO | 42000 | 100 | 4650 | 62.2 |