G88-40
taken from 2 paper(s):
/E.Caffau et al.(2005)/
/C.J.Hansen et al.(2012)/
Sulphur abundance in Galactic stars
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
S I | N/A | -0.62+-0.16 | 0.18+-0.16 | ... | -0.41+-0.16 | 0.39+-0.16 | 6.71+-0.16 | S I |
Fe | N/A | -0.80 | ... | ... | -0.80 | ... | 6.70 | Fe |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2450086.70663 | EMMIESO | 60000 | 120 | N/A | N/A |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 5929+-100 | log g : 4.14+-0.25 | vturb : 1.4+-0.15 |
Chemical Abundances
| | 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 | -0.89+-0.15 | ... | ... | -0.89+-0.15 | ... | 6.61+-0.15 | Fe |
Sr | N/A | ... | 0.04+-0.10 | ... | -0.85+-0.10 | 0.04+-0.10 | 2.02+-0.10 | Sr |
Y | N/A | ... | -0.27+-0.15 | ... | -1.16+-0.15 | -0.27+-0.15 | 1.05+-0.15 | Y |
Zr | N/A | ... | 0.02+-0.17 | ... | -0.87+-0.17 | 0.02+-0.17 | 1.71+-0.17 | Zr |
Pd | N/A | ... | 0.12+-0.19 | ... | -0.77+-0.19 | 0.12+-0.19 | 0.80+-0.19 | Pd |
Ag | N/A | ... | 0.03+-0.26 | ... | -1.12+-0.26 | -0.23+-0.26 | 0.08+-0.26 | Ag |
Ba | N/A | ... | 0.05+-0.14 | ... | -0.84+-0.14 | 0.05+-0.14 | 1.34+-0.14 | Ba |
Eu | N/A | ... | 0.32+-0.16 | ... | -0.57+-0.16 | 0.32+-0.16 | -0.05+-0.16 | Eu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >100 | N/A | N/A |