HD3567
taken from 12 paper(s):
/P.E.Nissen et al.(2002)/
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
/M.Asplund et al.(2006)/
/J.P.Fulbright(2000)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2009)/
/C.J.Hansen et al.(2012)/
/H.L.Yan et al.(2016)/
/B.E.Reddy et al.(2006)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
O/Fe in metal-poor main sequence and subgiant stars
Stellar Parameters
Teff : 6000 | log g : 4.07 | vturb : 1.5 |
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 | ... | 0.42+0.08-0.10 | 8.00+0.08-0.10 | -0.69+0.08-0.10 | 0.44+0.08-0.10 | 8.00+0.08-0.10 | [O I] |
Fe | N/A | -1.16 | ... | ... | -1.13 | ... | 6.37 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-04 | N/A | VLT | 55000 | 300-400 | N/A | N/A |
Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution
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 |
Fe | N/A | -1.2 | ... | ... | -1.20 | ... | 6.30 | Fe |
Cu I | N/A | ... | -0.66+-0.13 | ... | -1.84+-0.13 | -0.64+-0.13 | 2.35+-0.13 | Cu I |
Zn I | N/A | ... | -0.23+-0.16 | ... | -1.39+-0.16 | -0.19+-0.16 | 3.17+-0.16 | Zn I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
Analysis of neutron capture elements in metal-poor stars
Stellar Parameters
Teff : 5950 | log g : 3.8 | vturb : 0.5 |
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 |
Mg I | N/A | ... | -0.06 | ... | -1.28 | -0.08 | 6.32 | Mg I |
Si I | N/A | ... | 0.21 | ... | -0.95 | 0.25 | 6.56 | Si I |
Ca I | N/A | ... | 0.41 | ... | -0.77 | 0.43 | 5.57 | Ca I |
Fe | N/A | -1.20 | ... | ... | -1.20 | ... | 6.30 | Fe |
Sr I | N/A | ... | 0.37 | ... | -0.73 | 0.47 | 2.14 | Sr I |
Ba II | N/A | ... | 0.27 | ... | -0.98 | 0.22 | 1.20 | Ba II |
Ce II | N/A | ... | 0.23 | ... | -0.97 | 0.23 | 0.61 | Ce II |
Nd II | N/A | ... | 0.30 | ... | -0.82 | 0.38 | 0.60 | Nd II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
Lithium Isotopic Abundances in Metal-poor Halo Stars
Stellar Parameters
Teff : 6026 | log g : 4.08 | vturb : 1.5 |
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+-0.01 | -0.94+-0.01 | 0.20+-0.01 | 2.32+-0.01 | Li |
O | N/A | -0.79 | ... | ... | -0.74 | 0.40 | 7.95 | O |
Fe | N/A | -1.14 | ... | ... | -1.14 | ... | 6.36 | Fe |
Isotopic Ratio
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07-24-0843 | N/A | VLT | 120000 | 560 | 45 | -47.3 |
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 5950 | log g : 3.9 | vturb : 1.4 |
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 I | N/A | ... | ... | 2.3 | -0.96 | 0.34 | 2.3 | Li I |
Na I | N/A | ... | -0.17 | ... | -1.40 | -0.10 | 4.84 | Na I |
Mg I | N/A | ... | 0.27 | ... | -1.07 | 0.23 | 6.53 | Mg I |
Si I | N/A | ... | 0.34 | ... | -0.94 | 0.36 | 6.57 | Si I |
Ca I | N/A | ... | 0.33 | ... | -0.97 | 0.33 | 5.37 | Ca I |
Ti | N/A | ... | 0.31 | ... | -0.97 | 0.33 | 3.98 | Ti |
V I | N/A | ... | 0.09 | ... | -1.16 | 0.14 | 2.77 | V I |
Cr I | N/A | ... | -0.01 | ... | -1.30 | 0.00 | 4.34 | Cr I |
Fe | N/A | -1.32 | ... | ... | -1.30 | ... | 6.20 | Fe |
Ni I | N/A | ... | -0.05 | ... | -1.34 | -0.04 | 4.88 | Ni I |
Y II | N/A | ... | -0.06 | ... | -1.35 | -0.05 | 0.86 | Y II |
Zr II | N/A | ... | 0.23 | ... | -1.07 | 0.23 | 1.51 | Zr II |
Ba II | N/A | ... | 0.15 | ... | -1.22 | 0.08 | 0.96 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-08-08 | N/A | LICKHAMILTON | 50000 | 120 | 1800 | N/A |
Abundances for metal-poor stars with accurate parallaxes I. Basic data
Stellar Parameters
Teff : 6087 | log g : 4.16 | vturb : 0.98 |
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 | ... | 0.46+-0.069 | ... | -0.69+-0.069 | 0.54+-0.069 | 8.00+-0.069 | O I |
Na I | N/A | ... | -0.28+-0.054 | ... | -1.53+-0.054 | -0.30+-0.054 | 4.71+-0.054 | Na I |
Mg I | N/A | ... | 0.22+-0.055 | ... | -1.17+-0.055 | 0.06+-0.055 | 6.43+-0.055 | Mg I |
Si I | N/A | ... | 0.17+-0.048 | ... | -1.03+-0.048 | 0.20+-0.048 | 6.48+-0.048 | Si I |
Ca I | N/A | ... | 0.32+-0.033 | ... | -0.97+-0.033 | 0.26+-0.033 | 5.37+-0.033 | Ca I |
Ti I | N/A | ... | 0.17+-0.03 | ... | -0.93+-0.03 | 0.30+-0.03 | 4.02+-0.03 | Ti I |
Ti II | N/A | ... | 0.27+-0.048 | ... | -0.83+-0.048 | 0.40+-0.048 | 4.12+-0.048 | Ti II |
Fe I | N/A | -1.22+-0.051 | ... | ... | -1.23+-0.051 | ... | 6.27+-0.051 | Fe I |
Fe II | N/A | -1.26+-0.066 | ... | ... | -1.27+-0.066 | ... | 6.23+-0.066 | Fe II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 50000 | 200 | N/A | -49.7 |
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 5950 | log g : 4.1 | vturb : 1.4 |
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 | ... | ... | 2.42 | -0.84 | 0.36 | 2.42 | Li |
Be | N/A | ... | ... | -0.11 | -1.49 | -0.29 | -0.11 | Be |
Fe | N/A | -1.2 | ... | ... | -1.20 | ... | 6.30 | Fe |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 6035+-100 | log g : 4.08+-0.25 | vturb : 1.5+-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 | -1.33+-0.15 | ... | ... | -1.33+-0.15 | ... | 6.17+-0.15 | Fe |
Sr | N/A | ... | -0.1+-0.20 | ... | -1.43+-0.20 | -0.10+-0.20 | 1.44+-0.20 | Sr |
Y | N/A | ... | -0.18+-0.19 | ... | -1.51+-0.19 | -0.18+-0.19 | 0.70+-0.19 | Y |
Zr | N/A | ... | 0.27+-0.17 | ... | -1.06+-0.17 | 0.27+-0.17 | 1.52+-0.17 | Zr |
Pd | N/A | ... | 0.29+-0.20 | ... | -1.04+-0.20 | 0.29+-0.20 | 0.53+-0.20 | Pd |
Ag | N/A | ... | 0.53+-0.25 | ... | -1.06+-0.25 | 0.27+-0.25 | 0.14+-0.25 | Ag |
Ba | N/A | ... | 0.26+-0.17 | ... | -1.07+-0.17 | 0.26+-0.17 | 1.11+-0.17 | Ba |
Eu | N/A | ... | 0.70+-0.18 | ... | -0.63+-0.18 | 0.70+-0.18 | -0.11+-0.18 | Eu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >100 | N/A | N/A |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 6051 | log g : 4.02 | vturb : 1.5 |
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 | -1.16 | ... | ... | -1.16 | ... | 6.34 | Fe |
Cu | N/A | ... | -0.73+-0.00 | ... | -1.87+-0.00 | -0.71+-0.00 | 2.32+-0.00 | Cu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 55000 | 250-500 | N/A | N/A |
Elemental abundance survey of the Galactic thick disc
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 |
O | N/A | ... | 0.47 | ... | -0.53 | 0.56 | 8.16 | O |
Na | N/A | ... | 0.07 | ... | -0.94 | 0.15 | 5.30 | Na |
Mg | N/A | ... | 0.19 | ... | -0.91 | 0.18 | 6.69 | Mg |
Si | N/A | ... | 0.09 | ... | -0.84 | 0.25 | 6.67 | Si |
Ca | N/A | ... | 0.11 | ... | -0.94 | 0.15 | 5.40 | Ca |
Sc | N/A | ... | 0.13 | ... | -0.82 | 0.27 | 2.33 | Sc |
Ti | N/A | ... | 0.2 | ... | -0.89 | 0.20 | 4.06 | Ti |
Cr | N/A | ... | -0.21 | ... | -1.21 | -0.12 | 4.43 | Cr |
Mn | N/A | ... | -0.52 | ... | -1.62 | -0.53 | 3.81 | Mn |
Fe I | N/A | -1.04 | ... | ... | -1.09 | ... | 6.41 | Fe I |
Co | N/A | ... | 0.31 | ... | -0.79 | 0.30 | 4.20 | Co |
Ni | N/A | ... | -0.01 | ... | -1.04 | 0.05 | 5.18 | Ni |
Zn | N/A | ... | 0.03 | ... | -1.10 | -0.01 | 3.46 | Zn |
Y | N/A | ... | 0.06 | ... | -1.07 | 0.02 | 1.14 | Y |
Ba | N/A | ... | 0.09 | ... | -0.93 | 0.16 | 1.25 | Ba |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-06 | N/A | MCDONALD | 60000 | 100-200 | N/A | -50.2 |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 6051 | log g : 4.02 | vturb : 1.5 |
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 | ... | -0.24 | ... | -1.31 | -0.15 | 4.93 | Na |
Mg | N/A | ... | 0.14 | ... | -1.04 | 0.12 | 6.56 | Mg |
Si | N/A | ... | 0.17 | ... | -0.95 | 0.21 | 6.56 | Si |
Ca | N/A | ... | 0.31 | ... | -0.83 | 0.33 | 5.51 | Ca |
Ti | N/A | ... | 0.22 | ... | -0.87 | 0.29 | 4.08 | Ti |
Cr | N/A | ... | -0.05 | ... | -1.18 | -0.02 | 4.46 | Cr |
Fe | N/A | -1.16 | ... | ... | -1.16 | ... | 6.34 | Fe |
Ni | N/A | ... | -0.13 | ... | -1.26 | -0.10 | 4.96 | Ni |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-10-08-0419 | N/A | VLT | 55000 | 650 | N/A | -47.8 |
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 | ... | -0.33 | ... | -1.53 | -0.37 | 3.90 | Mn |
Fe | N/A | -1.16 | ... | ... | -1.16 | ... | 6.34 | Fe |
Cu | N/A | ... | -0.72 | ... | -1.86 | -0.70 | 2.33 | Cu |
Zn | N/A | ... | 0.01 | ... | -1.11 | 0.05 | 3.45 | Zn |
Y | N/A | ... | -0.05 | ... | -1.18 | -0.02 | 1.03 | Y |
Ba | N/A | ... | -0.09 | ... | -1.30 | -0.14 | 0.88 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-10-08-0419 | N/A | VLT | 55000 | 650 | N/A | -47.8 |