BPS CS22944-032: 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 |
1999-09-28 | N/A | KECKII | 7000 | 150 | 600 | N/A |
Binarity
Photometric data
V | 13.28 |
B-V | 0.59 |
EB-V | 0.04 |
Atmospheric data
Teff | 5528 |
log g | 3.44 |
vturb | -2.50 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -2.05 | 0.59 | 5.53 |
Ca I | ... | -2.42 | 0.22 | 3.94 |
Ti II | ... | -1.60 | 1.04 | 3.42 |
Fe I | ... | -2.64 | ... | 4.86 |
Ba II | ... | -3.22 | -0.58 | -1.09 |
: 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 | ... | -1.99+-0.26 | 0.65+-0.26 | 6.56+-0.26 |
Fe | ... | -2.64 | ... | 4.86 |
Sr | ... | -2.20 | 0.44 | 0.77 |
Ba | ... | -3.22 | -0.58 | -1.09 |
: 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 |
2004107-8 | N/A | KECKHIRES | N/A | 147 | 7200 | 17.7+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 5300+-100 |
log g | 2.87+-0.2 |
vturb | 1.5+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.67+-0.15 | 0.31+-0.15 | 5.88+-0.15 |
N | ... | <-3.42 | <-0.44 | <4.55 |
OH | ... | -2.23+-0.33 | 0.75+-0.33 | 6.64+-0.33 |
Mg | ... | -2.59+-0.09 | 0.39+-0.09 | 4.99+-0.09 |
Al | ... | -3.82+-0.16 | -0.84+-0.16 | 2.65+-0.16 |
Ca | ... | -2.69+-0.04 | 0.29+-0.04 | 3.67+-0.04 |
Sc II | ... | -2.87+-0.08 | 0.11+-0.08 | 0.30+-0.08 |
Ti I | ... | -2.66+-0.06 | 0.32+-0.06 | 2.36+-0.06 |
Ti II | ... | -2.62+-0.05 | 0.36+-0.05 | 2.40+-0.05 |
V II | ... | -2.82+-0.08 | 0.16+-0.08 | 1.18+-0.08 |
Cr I | ... | -3.29+-0.05 | -0.31+-0.05 | 2.38+-0.05 |
Mn I | ... | -3.42+-0.09 | -0.44+-0.09 | 1.97+-0.09 |
Mn II | ... | -3.17+-0.05 | -0.19+-0.05 | 2.22+-0.05 |
Fe I | ... | -2.98+-0.03 | ... | 4.52+-0.03 |
Fe II | ... | -3.04+-0.10 | ... | 4.46+-0.10 |
Co | ... | -2.53+-0.06 | 0.45+-0.06 | 2.39+-0.06 |
Ni | ... | -2.88+-0.06 | 0.10+-0.06 | 3.37+-0.06 |
Cu | ... | -4.08+-0.08 | -1.10+-0.08 | 0.13+-0.08 |
Zn | ... | -2.73+-0.17 | 0.25+-0.17 | 1.87+-0.17 |
Sr II | ... | -3.25+-0.08 | -0.27+-0.08 | -0.28+-0.08 |
Y II | ... | -3.28+-0.05 | -0.30+-0.05 | -1.04+-0.05 |
Zr II | ... | -2.93+-0.05 | 0.05+-0.05 | -0.33+-0.05 |
Ba II | ... | -3.60+-0.09 | -0.62+-0.09 | -1.47+-0.09 |
Eu II | ... | <-2.25 | <0.73 | <-1.74 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)