BPS CS22190-007: found in 3 paper(s).
Labels:
/D.K.Lai et al.(2004)/
/D.K.Lai et al.(2007)/
/G.W.Preston et al.(2006)/
Find this object in SIMBAD
D.K.Lai et al.,AJ, 128, 2402, 2004 (A0022,ADS)
Atmospheric data
Teff : 6013 | log g : 3.71 | vturb : -2.00 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -1.82 | 0.20 | 5.76 |
Ca I | ... | -1.91 | 0.11 | 4.45 |
Ti II | ... | -0.90 | 1.12 | 4.12 |
Fe I | ... | -2.02 | ... | 5.48 |
Ba II | ... | -1.11 | 0.91 | 1.02 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Binarity
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1999-11-30 | N/A | KECKII | 7000 | 150 | 900 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
Photometric data
V : 14.20 | B-V : 0.46 | EB-V : 0.03 |
D.K.Lai et al.,ApJ, 667, 1185, 2007 (A0128,ADS)
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.02+-0.26 | 0.00+-0.26 | 6.53+-0.26 |
Fe | ... | -2.02 | ... | 5.48 |
Sr | ... | -1.40 | 0.62 | 1.57 |
Ba | ... | -1.11 | 0.91 | 1.02 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | KECKII | 7000 | N/A | N/A | N/A |
G.W.Preston et al.,AJ, 132, 85, 2006 (A0182,ADS)
Atmospheric data
Teff : 5700+-150 | log g : 2.30+-0.3 | vturb : 1.95+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | <-2.70 | <-0.11 | <5.85 |
Na I | ... | -1.83+-0.07 | 0.76+-0.07 | 4.50+-0.07 |
Mg I | ... | -2.27+-0.07 | 0.32+-0.07 | 5.31+-0.07 |
Al I | ... | -3.47 | -0.88 | 3.00 |
Si I | ... | -2.32 | 0.27 | 5.23 |
Ca I | ... | -2.23+-0.08 | 0.36+-0.08 | 4.13+-0.08 |
Sc II | ... | -2.47+-0.11 | 0.12+-0.11 | 0.70+-0.11 |
Ti I | ... | -2.29+-0.14 | 0.30+-0.14 | 2.73+-0.14 |
Ti II | ... | -2.33+-0.09 | 0.26+-0.09 | 2.69+-0.09 |
V I | ... | -2.39 | 0.20 | 1.61 |
Cr I | ... | -2.76+-0.24 | -0.17+-0.24 | 2.91+-0.24 |
Cr II | ... | -2.46+-0.17 | 0.13+-0.17 | 3.21+-0.17 |
Mn I | ... | -3.21+-0.03 | -0.62+-0.03 | 2.18+-0.03 |
Fe I | ... | -2.59+-0.10 | ... | 4.91+-0.1 |
Fe II | ... | -2.55+-0.14 | ... | 4.95+-0.14 |
Sr II | ... | -2.39+-0.07 | 0.20+-0.07 | 0.58+-0.07 |
Y II | ... | -2.77+-0.14 | -0.18+-0.14 | -0.53+-0.14 |
Ba II | ... | -2.65+-0.1 | -0.06+-0.10 | -0.52+-0.1 |
La II | ... | -2.41+-0.15 | 0.18+-0.15 | -1.24+-0.15 |
Eu II | ... | -2.23+-0.15 | 0.36+-0.15 | -1.72+-0.15 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Binarity
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-18-0813 | N/A | MIKELCO | 40000 | 100 | 3600 | N/A |
Photometric data
V : 14.20 | B-V : 0.46 | U-B : -0.06 | V-K : 1.54 | EB-V : 0.00 |