G 166-37: found in 3 paper(s).
Labels:
/R.Smiljanic et al.(2006)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
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A0190
Title | Beryllium abundances and star formation in the halo and in the thick disk |
ADS | R.Smiljanic et al.,ApJ, 644, L121, 2006 |
Authors | R. Smiljanic, L. Pasquini, P. Bonifacio, D. Galli, R. G. Gratton, S. Randich, B. Wolff |
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Photometric data
Atmospheric data
Teff | 5300 |
log g | 4.69 |
vturb | 0.6 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | 0.12 | 1.32 | 1.28 |
Fe | ... | -1.2 | ... | 6.30 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0193
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 110 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 5350+-86 |
log g | 4.71+-0.36 |
vturb | 0.00+-0.50 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 0.04+-0.07 | 1.43+-0.07 | 1.20+-0.07 |
Fe | ... | -1.39+-0.10 | ... | 6.11+-0.10 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0199
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | 2450820.657 | KECKHIRES | 48000 | 110 | 1600 | 368.4+-0.7 |
Binarity
Photometric data
Atmospheric data
Teff | 5350+-86 |
log g | 4.71+-0.36 |
vturb | 0.00+-0.50 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -1.75+-0.10 | -0.35+-0.13 | 4.58+-0.10 |
Mg I | ... | -1.19+-0.05 | +0.21+-0.10 | 6.39+-0.05 |
Si | ... | -1.24+-0.10 | +0.16+-0.10 | 6.31+-0.10 |
Si I | ... | -1.24+-0.06 | 0.16+-0.06 | 6.31+-0.06 |
Ca I | ... | -1.20+-0.10 | +0.21+-0.13 | 5.16+-0.10 |
Ti | ... | -1.18+-0.11 | +0.22+-0.11 | 3.84+-0.11 |
Ti I | ... | -1.21+-0.09 | 0.19+-0.09 | 3.81+-0.09 |
Ti II | ... | -1.10+-0.14 | 0.30+-0.14 | 3.92+-0.14 |
Cr | ... | -1.36+-0.10 | +0.04+-0.10 | 4.31+-0.10 |
Cr I | ... | -1.45+-0.09 | -0.05+-0.09 | 4.22+-0.09 |
Cr II | ... | -1.28+-0.09 | 0.12+-0.09 | 4.39+-0.09 |
Fe | ... | -1.40+-0.08 | ... | 6.10+-0.08 |
Fe I | ... | -1.38+-0.09 | ... | 6.12+-0.09 |
Fe II | ... | -1.46+-0.16 | ... | 6.04+-0.16 |
Ni I | ... | -1.56+-0.07 | -0.16+-0.11 | 4.69+-0.07 |
Y II | ... | -1.28+-0.05 | +0.12+-0.09 | 0.96+-0.05 |
Ba II | ... | -1.26+-0.08 | +0.14+-0.11 | 0.87+-0.08 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)