BPS CS22957-022: found in 3 paper(s).
Labels:
/D.K.Lai et al.(2004)/
/D.K.Lai et al.(2007)/
/D.K.Lai et al.(2008)/
Find this object in SIMBAD
A0022
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-08-28 | N/A | KECKII | 7000 | 150 | 900 | N/A |
Binarity
Photometric data
Atmospheric data
Teff | 5075 |
log g | 2.41 |
vturb | -3.00 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -2.47 | 0.55 | 5.11 |
Ca I | ... | -2.58 | 0.44 | 3.78 |
Ti II | ... | -2.67 | 0.35 | 2.35 |
Fe I | ... | -3.02 | ... | 4.48 |
Ba II | ... | -3.91 | -0.89 | -1.78 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0128
Get more information of this paper.
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 | ... | -2.72+-0.22 | 0.30+-0.22 | 5.83+-0.22 |
Fe | ... | -3.02 | ... | 4.48 |
Sr | ... | -3.30 | -0.28 | -0.33 |
Ba | ... | -3.91 | -0.89 | -1.78 |
: 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 |
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-10-08 | N/A | KECKHIRES | N/A | 95 | 3600 | -33.8+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 5163+-100 |
log g | 2.47+-0.2 |
vturb | 1.6+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.77+-0.23 | 0.16+-0.23 | 5.78+-0.23 |
N | ... | -2.72+-0.23 | 0.21+-0.23 | 5.25+-0.23 |
OH | ... | -2.33+-0.33 | 0.60+-0.33 | 6.54+-0.33 |
Mg | ... | -2.65+-0.10 | 0.28+-0.10 | 4.93+-0.10 |
Ca | ... | -2.71+-0.04 | 0.22+-0.04 | 3.65+-0.04 |
Sc II | ... | -2.88+-0.06 | 0.05+-0.06 | 0.29+-0.06 |
Ti I | ... | -2.63+-0.06 | 0.30+-0.06 | 2.39+-0.06 |
Ti II | ... | -2.60+-0.05 | 0.33+-0.05 | 2.42+-0.05 |
V I | ... | -3.02+-0.16 | -0.09+-0.16 | 0.98+-0.16 |
V II | ... | -2.89+-0.08 | 0.04+-0.08 | 1.11+-0.08 |
Cr I | ... | -3.23+-0.05 | -0.30+-0.05 | 2.44+-0.05 |
Mn I | ... | -3.69+-0.10 | -0.76+-0.10 | 1.70+-0.10 |
Mn II | ... | -3.18+-0.05 | -0.25+-0.05 | 2.21+-0.05 |
Fe I | ... | -2.93+-0.03 | ... | 4.57+-0.03 |
Fe II | ... | -2.92+-0.10 | ... | 4.58+-0.10 |
Co | ... | -2.64+-0.09 | 0.29+-0.09 | 2.28+-0.09 |
Ni | ... | -2.95+-0.08 | -0.02+-0.08 | 3.30+-0.08 |
Cu | ... | -4.16+-0.09 | -1.23+-0.09 | 0.05+-0.09 |
Zn | ... | -2.62+-0.08 | 0.31+-0.08 | 1.98+-0.08 |
Sr II | ... | -3.34+-0.16 | -0.41+-0.16 | -0.37+-0.16 |
Y II | ... | -3.30+-0.06 | -0.37+-0.06 | -1.06+-0.06 |
Zr II | ... | -2.98+-0.08 | -0.05+-0.08 | -0.38+-0.08 |
Ba II | ... | -3.94+-0.10 | -1.01+-0.10 | -1.81+-0.10 |
Eu II | ... | <-3.02 | <-0.09 | <-2.51 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)