BPS CS22963-004: found in 3 paper(s).
Labels:
/D.K.Lai et al.(2004)/
/D.K.Lai et al.(2007)/
/D.K.Lai et al.(2008)/
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A0022
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1999-11-26 | N/A | KECKII | 7000 | 150 | 600 | N/A |
Binarity
Photometric data
V | 14.98 |
B-V | 0.53 |
EB-V | 0.05 |
Atmospheric data
Teff | 5803 |
log g | 3.61 |
vturb | -3.00 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -2.77 | 0.26 | 4.81 |
Ca I | ... | -2.77 | 0.26 | 3.59 |
Ti II | ... | -2.76 | 0.27 | 2.26 |
Fe I | ... | -3.03 | ... | 4.47 |
Ba II | ... | -3.30 | -0.27 | -1.17 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0128
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | KECKII | 7000 | N/A | N/A | N/A |
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | <-2.08 | <0.95 | <6.47 |
Fe | ... | -3.03 | ... | 4.47 |
Sr | ... | <-4.00 | <-0.97 | <-1.03 |
Ba | ... | <-3.30 | <-0.27 | <-1.17 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0181
Title | Detailed Abundances for 28 Metal-poor Stars: Stellar Relics in the Milky Way |
ADS | D.K.Lai et al.,ApJ, 681, 1524, 2008 |
Authors | D. K. Lai, M. Bolte, J. A. Johnson, S. Lucatello |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-10-08 | N/A | KECKHIRES | N/A | 71 | 9000 | 292.4+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 5659+-100 |
log g | 3.40+-0.2 |
vturb | 1.6+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.02+-0.23 | 0.40+-0.23 | 5.53+-0.23 |
N | ... | -2.62+-0.23 | 0.80+-0.23 | 5.35+-0.23 |
OH | ... | -2.43+-0.33 | 0.99+-0.33 | 6.44+-0.33 |
Mg | ... | -3.07+-0.10 | 0.35+-0.10 | 4.51+-0.10 |
Al | ... | -4.27+-0.16 | -0.85+-0.16 | 2.20+-0.16 |
Si | ... | -3.00+-0.21 | 0.42+-0.21 | 4.55+-0.21 |
Ca | ... | -3.11+-0.06 | 0.31+-0.06 | 3.25+-0.06 |
Sc II | ... | -3.15+-0.10 | 0.27+-0.10 | 0.02+-0.10 |
Ti II | ... | -2.98+-0.08 | 0.44+-0.08 | 2.04+-0.08 |
V II | ... | -3.35+-0.19 | 0.07+-0.19 | 0.65+-0.19 |
Cr I | ... | -3.82+-0.05 | -0.40+-0.05 | 1.85+-0.05 |
Mn I | ... | -4.19+-0.10 | -0.77+-0.10 | 1.20+-0.10 |
Mn II | ... | -3.84+-0.18 | -0.42+-0.18 | 1.55+-0.18 |
Fe I | ... | -3.42+-0.03 | ... | 4.08+-0.03 |
Fe II | ... | -3.44+-0.13 | ... | 4.06+-0.13 |
Co | ... | -2.94+-0.07 | 0.48+-0.07 | 1.98+-0.07 |
Ni | ... | -3.34+-0.07 | 0.08+-0.07 | 2.91+-0.07 |
Cu | ... | -4.36+-0.09 | -0.94+-0.09 | -0.15+-0.09 |
Sr II | ... | -4.22+-0.10 | -0.80+-0.10 | -1.25+-0.10 |
Ba II | ... | -3.86+-0.19 | -0.44+-0.19 | -1.73+-0.19 |
Eu II | ... | <-1.99 | <1.43 | <-1.48 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)