BD-01_306: found in 3 paper(s).
Labels:
/J.Simmerer et al.(2004)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2006)/
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A0131
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Atmospheric data
Teff | 5550 |
log g | 4.19 |
vturb | 1.50 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -1.28 | -0.15 | 7.27 |
Fe I | ... | -1.13 | ... | 6.37 |
Fe II | ... | -1.13 | ... | 6.37 |
La II | ... | -1.05+-0.04 | 0.08+-0.04 | 0.12+-0.04 |
Eu II | ... | -0.78+-0.08 | 0.35+-0.08 | -0.27+-0.08 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0135
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | N/A | 50000 | >100 | N/A | 19.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | -11205 |
Right Ascension | 21440 |
Photometric data
Atmospheric data
Teff | 5726 |
log g | 4.41 |
vturb | 0.8 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -0.96+-0.054 | -0.05+-0.054 | 5.37+-0.054 |
Mg I | ... | -0.43+-0.055 | 0.48+-0.055 | 7.15+-0.055 |
Si I | ... | -0.65+-0.048 | 0.26+-0.048 | 6.90+-0.048 |
Ca I | ... | -0.62+-0.033 | 0.29+-0.033 | 5.74+-0.033 |
Ti I | ... | -0.69+-0.03 | 0.22+-0.03 | 4.33+-0.03 |
Ti II | ... | -0.75+-0.048 | 0.16+-0.048 | 4.27+-0.048 |
Fe I | ... | -0.91+-0.051 | ... | 6.59+-0.051 |
Fe II | ... | -1.03+-0.066 | ... | 6.47+-0.066 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
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 | 5640 |
log g | 4.38 |
vturb | 1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | -0.16 | 0.64 | 1 |
Be | ... | -0.46 | 0.34 | 0.69 |
Fe | ... | -0.8 | ... | 6.70 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)