HE0134-2504
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
| Teff : 5204+-100 | log g : 2.5+-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 | ... | 1.79 | ... | -0.79 | 2.00 | 7.64 | CH |
| Na I | 3 | ... | 0.67+-0.15 | ... | -1.99+-0.15 | 0.80+-0.15 | 4.25+-0.15 | Na I |
| Mg I | 2 | ... | 0.46+-0.07 | ... | -2.34+-0.07 | 0.45+-0.07 | 5.26+-0.07 | Mg I |
| K I | 1 | ... | 0.43 | ... | -2.22 | 0.57 | 2.81 | K I |
| Ca I | 2 | ... | 0.16+-0.18 | ... | -2.56+-0.18 | 0.23+-0.18 | 3.78+-0.18 | Ca I |
| Ti I | 3 | ... | 0.39+-0.1 | ... | -2.31+-0.1 | 0.48+-0.1 | 2.64+-0.1 | Ti I |
| Ti II | 2 | ... | 0.21+-0.12 | ... | -2.49+-0.12 | 0.30+-0.12 | 2.46+-0.12 | Ti II |
| Cr I | 1 | ... | -0.43 | ... | -3.14 | -0.35 | 2.50 | Cr I |
| Fe I | N/A | -2.74+-0.15 | ... | ... | -2.79+-0.15 | ... | 4.71+-0.15 | Fe I |
| Fe II | 5 | -2.66+-0.15 | 0.08+-0.15 | ... | -2.71+-0.15 | 0.08+-0.15 | 4.79+-0.15 | Fe II |
| Sr II | 1 | ... | 0.97 | ... | -1.74 | 1.05 | 1.13 | Sr II |
| Y II | 3 | ... | 1.13+-0.29 | ... | -1.58+-0.29 | 1.21+-0.29 | 0.63+-0.29 | Y II |
| Ba II | 3 | ... | 1.65+-0.06 | ... | -1.14+-0.06 | 1.65+-0.06 | 1.04+-0.06 | Ba II |
| La II | 3 | ... | 1.37+-0.04 | ... | -1.33+-0.04 | 1.46+-0.04 | -0.23+-0.04 | La II |
| Ce II | 1 | ... | 1.66 | ... | -1.11 | 1.68 | 0.47 | Ce II |
| Vrad | 9 |
| Right Ascension : 01 36 37.30 | Declination : -24 49 03.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2004-09 | N/A | MIKELCO | 42000 | 71 | 1500 | 9 |