G183-11
taken from 3 paper(s):
/P.E.Nissen et al.(2002)/
/K.F.Tan et al.(2009)/
/C.J.Hansen et al.(2012)/
O/Fe in metal-poor main sequence and subgiant stars
Stellar Parameters
Teff : 6092 | log g : 4.04 | vturb : 1.5 |
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 | -2.10 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-04 | N/A | VLT | 55000 | 300-400 | N/A | N/A |
Beryllium abundances in metal-poor stars
Stellar Parameters
Teff : 6190+-80 | log g : 4.09+-0.15 | vturb : 1.5+-0.2 |
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 |
Li | N/A | ... | ... | 2.21 | -1.05 | 1.02 | 2.21 | Li |
Be | N/A | ... | ... | -0.61+-0.14 | -1.99+-0.14 | 0.08+-0.14 | -0.61+-0.14 | Be |
O | N/A | -1.27 | ... | ... | -1.19 | 0.88 | 7.50 | O |
Fe | N/A | -2.08 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-04-10 | N/A | VLT | 48000 | N/A | N/A | N/A |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 6309+-100 | log g : 3.97+-0.25 | vturb : 1.0+-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 | -2.12+-0.15 | ... | ... | -2.12+-0.15 | ... | 5.38+-0.15 | Fe |
Y | N/A | ... | -0.24+-0.12 | ... | -2.36+-0.12 | -0.24+-0.12 | -0.15+-0.12 | Y |
Zr | N/A | ... | 0.18+-0.17 | ... | -1.94+-0.17 | 0.18+-0.17 | 0.64+-0.17 | Zr |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >100 | N/A | N/A |