G88-32
taken from 4 paper(s):
/P.E.Nissen et al.(2002)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/C.J.Hansen et al.(2012)/
O/Fe in metal-poor main sequence and subgiant stars
Stellar Parameters
Teff : 6251 | log g : 3.81 | 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 | -2.41 | ... | ... | -2.38 | ... | 5.12 | 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 |
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 6136+-71 | log g : 3.54+-0.37 | vturb : 1.59+-0.16 |
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 I | N/A | ... | ... | 2.17+-0.06 | -1.09+-0.06 | 1.45+-0.06 | 2.17+-0.06 | Li I |
Fe | N/A | -2.56+-0.07 | ... | ... | -2.54+-0.07 | ... | 4.96+-0.07 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 120 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 6136+-71 | log g : 3.54+-0.37 | vturb : 1.59+-0.16 |
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 |
Mg I | N/A | -2.02+-0.16 | +0.53+-0.17 | ... | -2.04+-0.16 | 0.50+-0.17 | 5.56+-0.16 | Mg I |
Ca I | N/A | -2.18+-0.06 | +0.37+-0.09 | ... | -2.16+-0.06 | 0.38+-0.09 | 4.18+-0.06 | Ca I |
Ti | N/A | ... | +0.46+-0.09 | ... | -2.05+-0.09 | 0.49+-0.09 | 2.90+-0.09 | Ti |
Ti I | 3 | -2.10+-0.08 | ... | ... | -2.06+-0.08 | 0.48+-0.08 | 2.89+-0.08 | Ti I |
Ti II | 5 | -2.08+-0.10 | ... | ... | -2.04+-0.10 | 0.50+-0.10 | 2.91+-0.10 | Ti II |
Cr | N/A | ... | +0.00+-0.16 | ... | -2.52+-0.16 | 0.02+-0.16 | 3.12+-0.16 | Cr |
Cr I | 4 | -2.54+-0.14 | ... | ... | -2.51+-0.14 | 0.03+-0.14 | 3.13+-0.14 | Cr I |
Fe | N/A | -2.55+-0.06 | ... | ... | -2.54+-0.06 | ... | 4.96+-0.06 | Fe |
Fe I | 28 | -2.55+-0.07 | ... | ... | -2.54+-0.07 | ... | 4.96+-0.07 | Fe I |
Fe II | 9 | -2.54+-0.13 | ... | ... | -2.53+-0.13 | ... | 4.97+-0.13 | Fe II |
Ni I | N/A | -2.45+-0.16 | +0.10+-0.17 | ... | -2.42+-0.16 | 0.12+-0.17 | 3.80+-0.16 | Ni I |
Ba II | N/A | -2.96+-0.13 | -0.42+-0.15 | ... | -3.01+-0.13 | -0.47+-0.15 | -0.83+-0.13 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2450820.346 | KECKHIRES | 48000 | 120 | 300 | -237.7+-0.6 |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 6327+-100 | log g : 3.65+-0.25 | vturb : 1.5+-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 | -2.53+-0.15 | ... | ... | -2.53+-0.15 | ... | 4.97+-0.15 | Fe |
Y | N/A | ... | -0.14+-0.13 | ... | -2.67+-0.13 | -0.14+-0.13 | -0.46+-0.13 | Y |
Zr | N/A | ... | 0.25+-0.14 | ... | -2.28+-0.14 | 0.25+-0.14 | 0.30+-0.14 | Zr |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >100 | N/A | N/A |