BD+13_2698: found in 3 paper(s).
Labels:
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
/R.Smiljanic et al.(2006)/
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A0126
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998067-8 | N/A | LICKHAMILTON | N/A | 70 | 1200 | |
Photometric data
Atmospheric data
Teff | 5500 |
log g | 3.8 |
vturb | 1.05 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -0.81 | 0.16 | 5.52 |
Mg I | ... | -0.48 | 0.49 | 7.10 |
Al I | ... | -0.51 | 0.46 | 5.96 |
Si I | ... | -0.55 | 0.42 | 7.00 |
Ca I | ... | -0.63 | 0.34 | 5.73 |
Ti | ... | -0.72 | 0.25 | 4.30 |
V I | ... | -0.98 | -0.01 | 3.02 |
Cr I | ... | -0.92 | 0.05 | 4.75 |
Fe | ... | -0.97 | ... | 6.53 |
Ni I | ... | -0.89 | 0.08 | 5.36 |
Y II | ... | -1.07 | -0.1 | 1.17 |
Zr II | ... | -0.91 | 0.06 | 1.69 |
Ba II | ... | -1.03 | -0.06 | 1.10 |
Eu II | ... | -0.89 | 0.08 | -0.38 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
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 | 5705 |
log g | 3.69 |
vturb | 1.30 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -0.90 | ... | 6.60 |
Fe II | ... | -0.89 | ... | 6.61 |
La II | ... | -0.90+-0.05 | 0.00+-0.05 | 0.27+-0.05 |
Eu II | ... | -0.56+-0.04 | 0.34+-0.04 | -0.05+-0.04 |
: 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 | 5500 |
log g | 3.77 |
vturb | 1.05 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | -0.26 | 0.54 | 0.9 |
Be | ... | -0.78 | 0.02 | 0.37 |
Fe | ... | -0.8 | ... | 6.70 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)