A high-resolution spectral analysis of three carbon-enhanced metal-poor stars
| Teff : 4500 | log g : 1.0 | vturb : 2.0 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| C I | N/A | -0.49 | 1.57 | 7.9 | -0.53 | 1.58 | 7.9 | C I |
| Na I | N/A | -1.60 | +0.46 | 4.57 | -1.67 | 0.44 | 4.57 | Na I |
| Mg I | N/A | -1.48 | 0.58 | 6.05 | -1.55 | 0.56 | 6.05 | Mg I |
| Ca I | N/A | -1.96 | 0.1 | 4.35 | -1.99 | 0.12 | 4.35 | Ca I |
| Ti II | N/A | -1.55 | 0.49 | 3.35 | -1.60 | 0.51 | 3.35 | Ti II |
| Fe I | N/A | -2.06 | ... | 5.39+-0.13 | -2.11 | ... | 5.39+-0.13 | Fe I |
| Fe II | N/A | -2.04 | ... | 5.41+-0.18 | -2.09 | ... | 5.41+-0.18 | Fe II |
| Ni I | N/A | -2.53 | -0.47 | 3.7 | -2.52 | -0.41 | 3.7 | Ni I |
| Sr I | N/A | -0.67 | 1.39 | 2.25 | -0.62 | 1.49 | 2.25 | Sr I |
| Y II | N/A | -1.41 | 0.63 | 0.8 | -1.41 | 0.70 | 0.8 | Y II |
| Zr I | N/A | -0.49 | +1.57 | 2.10 | -0.48 | 1.63 | 2.10 | Zr I |
| Ba II | N/A | -0.22 | 1.82 | 1.95 | -0.23 | 1.88 | 1.95 | Ba II |
| La II | N/A | -0.28 | 1.76 | 0.85 | -0.25 | 1.86 | 0.85 | La II |
| Ce II | N/A | -0.17 | 1.87 | 1.75 | 0.17 | 2.28 | 1.75 | Ce II |
| Nd II | N/A | -0.5 | 1.54 | 0.95 | -0.47 | 1.64 | 0.95 | Nd II |
| Sm II | N/A | -0.36 | 1.68 | 0.65 | -0.31 | 1.80 | 0.65 | Sm II |
| Pb I | N/A | 0.15 | 2.21 | 2.15 | 0.11 | 2.22 | 2.15 | Pb I |
| Vrad | -244.9+-1.5 |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2003-3-25 | 2453544.12049 | SUBARUHDS | 50000 | N/A | 600 | N/A |
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +24 04 01.5 | Right Ascension : 00 54 13.61 |