HD210295: found in 3 paper(s).
Labels:
/J.P.Fulbright and J. A. Johnson(2003)/
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
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A0074
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-09-30 | N/A | GECKOCFHT | 130000 | 140 | 1800 | N/A |
2001-10-01 | N/A | GECKOCFHT | 130000 | N/A | 1800 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4700 |
log g | 2.31 |
vturb | 1.45 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O I | ... | -0.67+-0.09 | 0.56+-0.09 | 8.02+-0.13 |
Fe | ... | -1.23 | ... | 6.27 |
Fe I | ... | -1.42+-0.06 | ... | 6.08+-0.06 |
Fe II | ... | -1.21+-0.13 | ... | 6.29+-0.13 |
: 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 |
1998-08-10 | N/A | LICKHAMILTON | N/A | 85 | 2400 | |
Photometric data
Atmospheric data
Teff | 4800 |
log g | 2.2 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -1.14 | 0.20 | 0.02 |
Na I | ... | -1.39 | -0.05 | 4.94 |
Mg I | ... | -0.84 | 0.5 | 6.74 |
Al I | ... | -1.08 | 0.26 | 5.39 |
Si I | ... | -0.93 | 0.41 | 6.62 |
Ca I | ... | -1.11 | 0.23 | 5.25 |
Ti | ... | -1.05 | 0.29 | 3.97 |
V I | ... | -1.41 | -0.07 | 2.59 |
Cr I | ... | -1.44 | -0.1 | 4.23 |
Fe | ... | -1.34 | ... | 6.16 |
Ni I | ... | -1.42 | -0.08 | 4.83 |
Y II | ... | -1.30 | 0.04 | 0.94 |
Zr II | ... | -1.05 | 0.29 | 1.55 |
Ba II | ... | -1.33 | 0.01 | 0.80 |
Eu II | ... | -0.95 | 0.39 | -0.44 |
: 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 | 4750 |
log g | 2.50 |
vturb | 1.55 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -1.66 | -0.2 | 6.89 |
Fe I | ... | -1.46 | ... | 6.04 |
Fe II | ... | -1.25 | ... | 6.25 |
La II | ... | -1.27+-0.11 | 0.19+-0.11 | -0.1+-0.11 |
Eu II | ... | -0.85+-0.09 | 0.61+-0.09 | -0.34+-0.09 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)