HIP69788
Does the i-process operate at nearly solar metallicity?
| Teff : 5127+-11 | log g : 3.90+-0.14 | vturb : 0.61+-0.10 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Fe | N/A | -0.04+-0.04 | ... | ... | -0.04+-0.04 | ... | 7.46+-0.04 | Fe |
| Pr II | N/A | ... | 0.02+-0.14 | 0.70 | -0.02 | 0.02+-0.14 | 0.70 | Pr II |
| Nd II | N/A | ... | -0.18+-0.10 | 1.20 | -0.22 | -0.18+-0.10 | 1.20 | Nd II |
| Sm II | N/A | ... | 0.08+-0.09 | 1.00 | 0.04 | 0.08+-0.09 | 1.00 | Sm II |
| Eu II | N/A | ... | -0.28+-0.09 | 0.20 | -0.32 | -0.28+-0.09 | 0.20 | Eu II |
| Right Ascension : | Declination : | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| N/A | N/A | HERMES | 86000 | N/A | N/A | N/A |