HD18907: found in 4 paper(s).
Labels:
/J.P.Fulbright and J. A. Johnson(2003)/
/J.P.Fulbright(2000)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2006)/
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A0074
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-09-29 | N/A | GECKOCFHT | 130000 | 320 | 600 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 5.88 |
B-V | 0.74 |
EB-V | 0.05 |
Atmospheric data
Teff | 5175 |
log g | 3.6 |
vturb | 1.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O I | ... | -0.14+-0.03 | 0.59+-0.03 | 8.55+-0.03 |
Fe | ... | -0.73 | ... | 6.77 |
Fe I | ... | -0.57+-0.08 | ... | 6.93+-0.08 |
Fe II | ... | -0.71+-0.04 | ... | 6.79+-0.04 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0126
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-10-30 | N/A | LICKHAMILTON | N/A | 110 | 300 | |
Photometric data
Atmospheric data
Teff | 5075 |
log g | 3.6 |
vturb | 1.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -0.60 | 0.11 | 5.73 |
Mg I | ... | -0.28 | 0.43 | 7.30 |
Al I | ... | -0.28 | 0.43 | 6.19 |
Si I | ... | -0.33 | 0.38 | 7.22 |
Ca I | ... | -0.44 | 0.27 | 5.92 |
Ti | ... | -0.38 | 0.33 | 4.64 |
V I | ... | -0.54 | 0.17 | 3.46 |
Cr I | ... | -0.67 | 0.04 | 5.00 |
Fe | ... | -0.71 | ... | 6.79 |
Ni I | ... | -0.65 | 0.06 | 5.60 |
Y II | ... | -0.65 | 0.06 | 1.59 |
Zr II | ... | -0.33 | 0.38 | 2.27 |
Ba II | ... | -0.80 | -0.09 | 1.33 |
Eu II | ... | -0.32 | 0.39 | 0.19 |
: 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 | -38.4 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | -280530 |
Right Ascension | 30138 |
Photometric data
Atmospheric data
Teff | 5015 |
log g | 3.49 |
vturb | 1.41 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -0.64+-0.054 | 0.24+-0.054 | 5.69+-0.054 |
Mg I | ... | -0.33+-0.055 | 0.55+-0.055 | 7.25+-0.055 |
Si I | ... | -0.44+-0.048 | 0.44+-0.048 | 7.11+-0.048 |
Ca I | ... | -0.55+-0.033 | 0.33+-0.033 | 5.81+-0.033 |
Ti I | ... | -0.65+-0.03 | 0.23+-0.03 | 4.37+-0.03 |
Ti II | ... | -0.64+-0.048 | 0.24+-0.048 | 4.38+-0.048 |
Fe I | ... | -0.88+-0.051 | ... | 6.62+-0.051 |
Fe II | ... | -0.88+-0.066 | ... | 6.62+-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 | 5075 |
log g | 3.48 |
vturb | 1.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -0.6 | ... | 6.90 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)