G 5-19: 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 | 5942 |
log g | 4.24 |
vturb | 0.89 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | 1.10 | 2.20 | 2.26 |
Be | ... | -1.16 | -0.06 | -0.01 |
Fe | ... | -1.1 | ... | 6.40 |
: 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 | 5942+-56 |
log g | 4.24+-0.24 |
vturb | 0.89+-0.11 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 1.10+-0.05 | 2.20+-0.05 | 2.26+-0.05 |
Fe | ... | -1.10+-0.08 | ... | 6.40+-0.08 |
: 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 | 2451067.648 | KECKHIRES | 48000 | 110 | 200 | -215.6+-0.6 |
Binarity
Photometric data
Atmospheric data
Teff | 5942+-56 |
log g | 4.24+-0.24 |
vturb | 0.89+-0.11 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -1.37+-0.20 | -0.21+-0.20 | 4.96+-0.20 |
Mg I | ... | -0.96+-0.09 | +0.20+-0.10 | 6.62+-0.09 |
Si | ... | -1.04+-0.10 | +0.12+-0.10 | 6.51+-0.10 |
Si I | ... | -0.97+-0.12 | 0.19+-0.12 | 6.58+-0.12 |
Si II | ... | -1.17+-0.16 | -0.01+-0.16 | 6.38+-0.16 |
Ca I | ... | -0.97+-0.08 | +0.19+-0.09 | 5.39+-0.08 |
Ti | ... | -0.94+-0.09 | +0.22+-0.09 | 4.08+-0.09 |
Ti I | ... | -1.00+-0.12 | 0.16+-0.12 | 4.02+-0.12 |
Ti II | ... | -0.90+-0.10 | 0.26+-0.10 | 4.12+-0.10 |
Cr | ... | -1.16+-0.08 | +0.00+-0.08 | 4.51+-0.08 |
Cr I | ... | -1.18+-0.08 | -0.02+-0.08 | 4.49+-0.08 |
Cr II | ... | -1.06+-0.17 | 0.10+-0.17 | 4.61+-0.17 |
Fe | ... | -1.16+-0.04 | ... | 6.34+-0.04 |
Fe I | ... | -1.09+-0.08 | ... | 6.41+-0.08 |
Fe II | ... | -1.18+-0.05 | ... | 6.32+-0.05 |
Ni I | ... | -1.26+-0.13 | -0.10+-0.13 | 4.99+-0.13 |
Y II | ... | -1.21+-0.05 | -0.05+-0.07 | 1.03+-0.05 |
Ba II | ... | -1.01+-0.13 | +0.15+-0.14 | 1.12+-0.13 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)