BPS CS22944-032: found in 4 paper(s).
Labels:
/D.K.Lai et al.(2004)/
/D.K.Lai et al.(2007)/
/D.K.Lai et al.(2008)/
/I.U.Roederer et al.(2014)/
Find this object in SIMBAD
D.K.Lai et al.,AJ, 128, 2402, 2004 (A0022,ADS)
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)
Binarity
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1999-09-28 | N/A | KECKII | 7000 | 150 | 600 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
Photometric data
V : 13.28 | B-V : 0.59 | EB-V : 0.04 |
D.K.Lai et al.,ApJ, 667, 1185, 2007 (A0128,ADS)
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)
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | KECKII | 7000 | N/A | N/A | N/A |
D.K.Lai et al.,ApJ, 681, 1524, 2008 (A0181,ADS)
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+-0.1 |
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)
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004107-8 | N/A | KECKHIRES | 46000 | 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
I.U.Roederer et al.,AJ, 147, 136, 2014 (A0309,ADS)
Atmospheric data
Teff : 5090+-36 | log g : 2.3+-0.14 | vturb : 1.45+-0.06 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -3.22-0.15 | +-0.15 | 1 |
CH | ... | -3.01+-0.25 | 0.21+-0.25 | 5.49 |
NH | ... | <-3.27 | <-0.05 | <4.7 |
O I | ... | <-2.61 | <0.61 | <6.26 |
Mg I | ... | -2.68+-0.15 | 0.54+-0.15 | 4.93 |
Al I | ... | -4.04+-0.26 | -0.82+-0.26 | 2.41 |
Si I | ... | -2.38+-0.29 | 0.84+-0.29 | 5.13 |
Ca I | ... | -2.77+-0.17 | 0.45+-0.17 | 3.58 |
Sc II | ... | -3.27+-0.16 | -0.05+-0.16 | -0.05 |
Ti I | ... | -2.94+-0.15 | 0.28+-0.15 | 2.01 |
Ti II | ... | -3.00+-0.16 | 0.22+-0.16 | 2.01 |
V I | ... | -3.11+-0.18 | 0.11+-0.18 | 0.82 |
V II | ... | -3.09+-0.29 | 0.13+-0.29 | 0.91 |
Cr I | ... | -3.35+-0.15 | -0.13+-0.15 | 2.29 |
Cr II | ... | -3.12+-0.19 | 0.1+-0.19 | 2.59 |
Mn I | ... | -3.45+-0.17 | -0.23+-0.17 | 1.98 |
Mn II | ... | -3.54+-0.21 | -0.32+-0.21 | 1.96 |
Fe I | ... | -3.22+-0.15 | ... | 4.28 |
Fe II | ... | -3.15+-0.16 | ... | 4.35 |
Co I | ... | -3.04+-0.21 | 0.18+-0.21 | 1.95 |
Ni I | ... | -2.91+-0.22 | 0.31+-0.22 | 3.31 |
Zn I | ... | -2.92+-0.19 | 0.3+-0.19 | 1.65 |
Rb I | ... | <-0.65 | <2.57 | <1.95 |
Sr II | ... | -3.48+-0.22 | -0.26+-0.22 | -0.55 |
Y II | ... | -3.78+-0.2 | -0.56+-0.2 | -1.5 |
Zr II | ... | -3.28+-0.18 | -0.06+-0.18 | -0.63 |
Nb II | ... | <-0.92 | <2.30 | <0.5 |
Mo I | ... | <-2.16 | <1.06 | <-0.24 |
Tc I | ... | <0.25 | <3.47 | <0.25 |
Sn I | ... | <-0.80 | <2.42 | <1.2 |
Ba II | ... | -4.20+-0.16 | -0.98+-0.16 | -1.95 |
La II | ... | <-2.98 | <0.24 | <-1.81 |
Ce II | ... | <-2.81 | <0.41 | <-1.23 |
Pr II | ... | <-2.44 | <0.78 | <-1.73 |
Nd II | ... | <-3.07 | <0.15 | <-1.57 |
Sm II | ... | <-2.29 | <0.93 | <-1.28 |
Eu II | ... | <-3.29 | <-0.07 | <-2.78 |
Gd II | ... | <-2.16 | <1.06 | <-1.04 |
Tb II | ... | <-0.73 | <2.49 | <-0.83 |
Dy II | ... | <-3.07 | <0.15 | <-1.93 |
Ho II | ... | <-1.55 | <1.67 | <-1.29 |
Er II | ... | <-2.54 | <0.68 | <-1.61 |
Tm II | ... | <-1.91 | <1.31 | <-1.91 |
Yb II | ... | -3.84+-0.56 | -0.62+-0.56 | -2.85 |
Hf II | ... | <-1.63 | <1.59 | <-0.75 |
Ir I | ... | <-1.10 | <2.12 | <0.25 |
Pb I | ... | <-1.24 | <1.98 | <0.71 |
Th II | ... | <-1.69 | <1.53 | <-1.69 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Binarity
Binarity | Negative |
Vrad | 19 |
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-06-30-09:51 | 2453186.915 | MIKELCO | 41000 | 145-235 | 4400 | 19.3 |
2007-08-22-03:12 | 2454334.639 | MIKELCO | 41000 | 145-235 | 800 | 18.5 |
2007-08-23-02:35 | 2454335.613 | MIKELCO | 41000 | 145-235 | 2000 | 19.1 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
Photometric data
V : 13.28 | B-V : 0.55 | V-K : 1.84 | EB-V : 0.043 |