HD241253: found in 3 paper(s).
Labels:
/R.G.Gratton et al.(2003)/
/E.Caffau et al.(2005)/
/R.Smiljanic et al.(2006)/
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A0135
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | EMMIESO | 60000 | 150 | N/A | -16 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | 53327 |
Right Ascension | 50957 |
Binarity
Photometric data
Atmospheric data
Teff | 5897 |
log g | 4.33 |
vturb | 0.55 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O I | ... | -0.49+-0.069 | 0.59+-0.069 | 8.38+-0.069 |
Na I | ... | -1.10+-0.054 | -0.02+-0.054 | 5.23+-0.054 |
Mg I | ... | -0.66+-0.055 | 0.42+-0.055 | 6.92+-0.055 |
Si I | ... | -0.82+-0.048 | 0.26+-0.048 | 6.73+-0.048 |
Ca I | ... | -0.81+-0.033 | 0.27+-0.033 | 5.55+-0.033 |
Ti I | ... | -0.90+-0.03 | 0.18+-0.03 | 4.12+-0.03 |
Ti II | ... | -0.87+-0.048 | 0.21+-0.048 | 4.15+-0.048 |
Fe I | ... | -1.08+-0.051 | ... | 6.42+-0.051 |
Fe II | ... | -1.19+-0.066 | ... | 6.31+-0.066 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0137
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | 2450087.63413 | EMMIESO | 60000 | 150 | N/A | |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | 53327 |
Right Ascension | 50957 |
Binarity
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
S I | ... | -0.82+-0.13 | 0.26+-0.13 | 6.51+-0.13 |
Fe | ... | -1.08 | ... | 6.42 |
: 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 | 5700 |
log g | 4.26 |
vturb | 1.11 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | 0.92 | 2.12 | 2.08 |
Be | ... | -0.68 | 0.52 | 0.47 |
Fe | ... | -1.2 | ... | 6.30 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)