HD149414: found in 6 paper(s).
Labels:
/G.S.Bai et al.(2004)/
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
/D.Yong and D. L. Lambert(2003)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2006)/
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A0023
Title | Chemical abundances of 10 metal-poor halo stars |
ADS | G.S.Bai et al.,AAP, 425, 671, 2004 |
Authors | G. S. National Astronomical Observatories, ChineseAcademyofSciencea. Bai, G. Zhao, Y. Q. National Astronomical Observatories, ChineseAcademyofSciencea. Chen, J. R. National Astronomical Observatories, ChineseAcademyofSciencea. Shi, V. G. Special Astrophysical Observatory, RussianAcademyofSciences. Klochkova, V. E. Special Astrophysical Observatory, RussianAcademyofSciences. Panchuk, H. M. National Astronomical Observatories, ChineseAcademyofSciencea. Qiu, H. W. National Astronomical Observatories, ChineseAcademyofSciencea. Zhang |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-17 | N/A | PFESSAO | 15000 | 218 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 5090 |
log g | 4.60+-0.3 |
vturb | 1.50 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O I | ... | -0.82 | 0.69 | 8.05 |
Na I | ... | -1.96 | -0.45 | 4.37 |
Mg I | ... | -1.29 | 0.22 | 6.29 |
Si I | ... | -1.06 | 0.45 | 6.49 |
Ca I | ... | -1.06 | 0.45 | 5.30 |
Sc II | ... | -1.36 | 0.15 | 1.81 |
Ti | ... | -1.15 | 0.36 | 3.87 |
Cr | ... | -1.49 | 0.02 | 4.18 |
Mn I | ... | -1.74 | -0.23 | 3.65 |
Fe I | ... | -1.51 | ... | 5.99 |
Ba II | ... | -1.23 | 0.28 | 0.90 |
: 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 |
1995-06-10 | N/A | LICKHAMILTON | N/A | 105 | 2000 | |
Photometric data
Atmospheric data
Teff | 5175 |
log g | 4.7 |
vturb | 0.3 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -1.37 | -0.11 | 4.96 |
Mg I | ... | -0.85 | 0.41 | 6.73 |
Al I | ... | -1.06 | 0.2 | 5.41 |
Si I | ... | -0.91 | 0.35 | 6.64 |
Ca I | ... | -0.99 | 0.27 | 5.37 |
Ti | ... | -0.87 | 0.39 | 4.15 |
V I | ... | -1.12 | 0.14 | 2.88 |
Cr I | ... | -1.20 | 0.06 | 4.47 |
Fe | ... | -1.26 | ... | 6.24 |
Y II | ... | -0.89 | 0.37 | 1.35 |
Zr II | ... | -0.62 | 0.64 | 1.98 |
Ba II | ... | -1.20 | 0.06 | 0.93 |
Eu II | ... | -0.76 | 0.5 | -0.25 |
: 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 | 4966 |
log g | 4.26 |
vturb | 0.80 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -1.59 | -0.05 | 6.96 |
Fe I | ... | -1.54 | ... | 5.96 |
Fe II | ... | -1.44 | ... | 6.06 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0133
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MCDONALD | 60000 | 90 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | -041345 |
Right Ascension | 163442 |
Atmospheric data
Teff | 4950+-150 |
log g | 4.50+-0.3 |
vturb | 0.3+-0.3 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -1.46+-0.2 | ... | 6.04+-0.2 |
: 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 | -169.9 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | -41344 |
Right Ascension | 163443 |
Binarity
Photometric data
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -1.31+-0.054 | 0.07+-0.054 | 5.02+-0.054 |
Mg I | ... | -0.76+-0.055 | 0.62+-0.055 | 6.82+-0.055 |
Si I | ... | -0.92+-0.048 | 0.46+-0.048 | 6.63+-0.048 |
Ca I | ... | -1.02+-0.033 | 0.36+-0.033 | 5.34+-0.033 |
Ti I | ... | -1.03+-0.03 | 0.35+-0.03 | 3.99+-0.03 |
Ti II | ... | -1.07+-0.048 | 0.31+-0.048 | 3.95+-0.048 |
Fe I | ... | -1.38+-0.051 | ... | 6.12+-0.051 |
Fe II | ... | -1.34+-0.066 | ... | 6.16+-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 | 5175 |
log g | 4.64 |
vturb | 0.3 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | <-0.86 | <0.24 | <0.30 |
Be | ... | -0.57 | 0.53 | 0.58 |
Fe | ... | -1.1 | ... | 6.40 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)