CD-33_3337
taken from 7 paper(s):
/M.Asplund et al.(2006)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2009)/
/J.Melendez et al.(2010)/
/C.J.Hansen et al.(2012)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

M.Asplund et al.,ApJ, 644, 229, 2006 (A0089,ADS)
Lithium Isotopic Abundances in Metal-poor Halo Stars
Stellar Parameters
Teff : 5897 | log g : 4.01 | vturb : 1.3 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li | N/A | ... | ... | 2.23+-0.01 | -1.03+-0.01 | 0.28+-0.01 | 2.23+-0.01 | Li |
O | N/A | -0.76 | ... | ... | -0.71 | 0.60 | 7.98 | O |
Fe | N/A | -1.31 | ... | ... | -1.31 | ... | 6.19 | Fe |
Isotopic Ratio
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-05-0157 | N/A | VLT | 120000 | 740 | 30 | 73.7 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
R.G.Gratton et al.,AAP, 404, 187, 2003 (A0135,ADS)
Abundances for metal-poor stars with accurate parallaxes
Stellar Parameters
Teff : 6079 | log g : 4.03 | vturb : 0.7 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
O I | N/A | ... | 0.49+-0.069 | ... | -0.72+-0.069 | 0.57+-0.069 | 7.97+-0.069 | O I |
Na I | N/A | ... | 0.06+-0.054 | ... | -1.25+-0.054 | 0.04+-0.054 | 4.99+-0.054 | Na I |
Mg I | N/A | ... | 0.44+-0.055 | ... | -1.01+-0.055 | 0.28+-0.055 | 6.59+-0.055 | Mg I |
Si I | N/A | ... | 0.18+-0.048 | ... | -1.08+-0.048 | 0.21+-0.048 | 6.43+-0.048 | Si I |
Ca I | N/A | ... | 0.25+-0.033 | ... | -1.10+-0.033 | 0.19+-0.033 | 5.24+-0.033 | Ca I |
Ti I | N/A | ... | 0.26+-0.03 | ... | -0.90+-0.03 | 0.39+-0.03 | 4.05+-0.03 | Ti I |
Ti II | N/A | ... | 0.26+-0.048 | ... | -0.90+-0.048 | 0.39+-0.048 | 4.05+-0.048 | Ti II |
Fe I | N/A | -1.28+-0.051 | ... | ... | -1.29+-0.051 | ... | 6.21+-0.051 | Fe I |
Fe II | N/A | -1.35+-0.066 | ... | ... | -1.36+-0.066 | ... | 6.14+-0.066 | Fe II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | EMMIESO | 60000 | 150 | N/A | 67 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -334449 | Right Ascension : 65448 |
R.Smiljanic et al.,AAP, 499, 103, 2009 (A0190,ADS)
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 6097 | log g : 4 | vturb : 1.86 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li | N/A | ... | ... | 2.32 | -0.94 | 0.36 | 2.32 | Li |
Be | N/A | ... | ... | 0.33 | -1.05 | 0.25 | 0.33 | Be |
Fe | N/A | -1.3 | ... | ... | -1.30 | ... | 6.20 | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
J.Melendez et al.,AAP, 515, L3, 2010 (A0235,ADS)
Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion
Stellar Parameters
Teff : 6001+-50 | log g : 4.00 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li | N/A | ... | ... | 2.30+-0.035 | -0.96+-0.035 | 0.37+-0.035 | 2.30+-0.035 | Li |
Fe | N/A | -1.33 | ... | ... | -1.33 | ... | 6.17 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | FIESNOT | 35000 | N/A | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
C.J.Hansen et al.,AAP, 545, A31, 2012 (A0272,ADS)
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 5952+-100 | log g : 3.95+-0.25 | vturb : 1.4+-0.15 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -1.55+-0.15 | ... | ... | -1.55+-0.15 | ... | 5.95+-0.15 | Fe |
Sr | N/A | ... | 0.22+-0.11 | ... | -1.33+-0.11 | 0.22+-0.11 | 1.54+-0.11 | Sr |
Y | N/A | ... | 0.01+-0.13 | ... | -1.54+-0.13 | 0.01+-0.13 | 0.67+-0.13 | Y |
Zr | N/A | ... | 0.27+-0.17 | ... | -1.28+-0.17 | 0.27+-0.17 | 1.30+-0.17 | Zr |
Pd | N/A | ... | 0.19+-0.27 | ... | -1.36+-0.27 | 0.19+-0.27 | 0.21+-0.27 | Pd |
Ag | N/A | ... | 0.27+-0.25 | ... | -1.54+-0.25 | 0.01+-0.25 | -0.34+-0.25 | Ag |
Ba | N/A | ... | 0.18+-0.14 | ... | -1.37+-0.14 | 0.18+-0.14 | 0.81+-0.14 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P.E.Nissen et al.,AAP, 511, L10, 2010 (C0012,ADS)
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5979 | log g : 3.86 | vturb : 1.7 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na | N/A | ... | 0.13 | ... | -1.14 | 0.22 | 5.10 | Na |
Mg | N/A | ... | 0.32 | ... | -1.06 | 0.30 | 6.54 | Mg |
Si | N/A | ... | 0.28 | ... | -1.04 | 0.32 | 6.47 | Si |
Ca | N/A | ... | 0.3 | ... | -1.04 | 0.32 | 5.30 | Ca |
Ti | N/A | ... | 0.3 | ... | -0.99 | 0.37 | 3.96 | Ti |
Cr | N/A | ... | -0.02 | ... | -1.35 | 0.01 | 4.29 | Cr |
Fe | N/A | -1.36 | ... | ... | -1.36 | ... | 6.14 | Fe |
Ni | N/A | ... | 0.00 | ... | -1.33 | 0.03 | 4.89 | Ni |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-11-26-0743 | N/A | VLT | 55000 | 600 | N/A | 73.6 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P. E. Nissen et al.,AAP, 530, A15, 2011 (C0013,ADS)
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Mn | N/A | ... | -0.27 | ... | -1.67 | -0.31 | 3.76 | Mn |
Fe | N/A | -1.36 | ... | ... | -1.36 | ... | 6.14 | Fe |
Cu | N/A | ... | -0.22 | ... | -1.56 | -0.20 | 2.63 | Cu |
Zn | N/A | ... | 0.1 | ... | -1.22 | 0.14 | 3.34 | Zn |
Y | N/A | ... | -0.06 | ... | -1.39 | -0.03 | 0.82 | Y |
Ba | N/A | ... | -0.19 | ... | -1.60 | -0.24 | 0.58 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-11-26-0743 | N/A | VLT | 55000 | 600 | N/A | 73.6 |