CS22189-009
taken from 14 paper(s):
/R.Cayrel et al.(2004)/
/M.Spite et al.(2005)/
/A.McWilliam et al.(1995)/
/A.McWilliam et al.(1995)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/S.M.Andrievsky et al.(2008)/
/S.M.Andrievsky et al.(2009)/
/S.M.Andrievsky et al.(2010)/
/M.Spite et al.(2011)/
/P.Francois et al.(2007)/
/M.Spite et al.(2012)/
/I.U.Roederer et al.(2014)/
/K.A.Venn et al.(2004)/
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 |
CH | N/A | -3.22 | 0.27 | 5.30 | -3.13 | 0.36 | 5.30 | CH |
Na I | 2 | -3.79 | -0.30 | 2.54 | -3.70 | -0.21 | 2.54 | Na I |
Mg I | 7 | -3.38+-0.06 | 0.11+-0.06 | 4.20+-0.06 | -3.40+-0.06 | 0.09+-0.06 | 4.20+-0.06 | Mg I |
Al I | 2 | -4.41 | -0.92 | 2.06 | -4.39 | -0.90 | 2.06 | Al I |
Si I | 1 | -3.20 | 0.29 | 4.35 | -3.16 | 0.33 | 4.35 | Si I |
K I | 1 | -3.09 | 0.40 | 2.03 | -3.00 | 0.49 | 2.03 | K I |
Ca I | 15 | -3.29+-0.10 | 0.20+-0.10 | 3.07+-0.10 | -3.27+-0.10 | 0.22+-0.10 | 3.07+-0.10 | Ca I |
Sc II | 7 | -3.49+-0.08 | 0.00+-0.08 | -0.32+-0.08 | -3.47+-0.08 | 0.02+-0.08 | -0.32+-0.08 | Sc II |
Ti I | 14 | -3.36+-0.16 | 0.13+-0.16 | 1.66+-0.16 | -3.29+-0.16 | 0.20+-0.16 | 1.66+-0.16 | Ti I |
Ti II | 30 | -3.45+-0.11 | 0.04+-0.11 | 1.57+-0.11 | -3.38+-0.11 | 0.11+-0.11 | 1.57+-0.11 | Ti II |
Cr I | 7 | -3.91+-0.13 | -0.42+-0.13 | 1.76+-0.13 | -3.88+-0.13 | -0.39+-0.13 | 1.76+-0.13 | Cr I |
Mn I | 3 | -3.74+-0.05 | -0.25+-0.05 | 1.65+-0.05 | -3.78+-0.05 | -0.29+-0.05 | 1.65+-0.05 | Mn I |
Fe I | 150 | -3.49+-0.15 | 0.00+-0.15 | 4.01+-0.15 | -3.49+-0.15 | 0.00+-0.15 | 4.01+-0.15 | Fe I |
Fe II | 11 | -3.49+-0.11 | 0.00+-0.11 | 4.01+-0.11 | -3.49+-0.11 | 0.00+-0.11 | 4.01+-0.11 | Fe II |
Co I | 4 | -3.12+-0.06 | 0.37+-0.06 | 1.80+-0.06 | -3.19+-0.06 | 0.30+-0.06 | 1.80+-0.06 | Co I |
Ni I | 3 | -3.43+-0.06 | 0.06+-0.06 | 2.82+-0.06 | -3.40+-0.06 | 0.09+-0.06 | 2.82+-0.06 | Ni I |
Zn I | 1 | -3.03 | 0.46 | 1.57 | -2.99 | 0.50 | 1.57 | Zn I |
Binary Parameters
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-10 | N/A | VLT | 47000 | 90 | 7200 | N/A |
First stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 | ... | ... | 0.54+-0.05 | -2.72+-0.05 | 0.77+-0.05 | 0.54+-0.05 | Li I |
C | N/A | -3.18+-0.08 | ... | ... | -3.09+-0.08 | 0.40+-0.08 | 5.34+-0.08 | C |
N | N/A | -3.22 | ... | ... | -3.13 | 0.36 | 4.70 | N |
Fe | N/A | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 47000 | 30 | N/A | N/A |
A Spectroscopic Analysis of 33 of the Most Metal-Poor Stars.I.
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | FRUTTI | 22000 | N/A | N/A | N/A |
Spectroscopic Analysis of 33 of the Most Metal Poor Stars. II.
Stellar Parameters
Teff : 4860 | log g : 1.70+-0.29 | vturb : 2.28+-0.12 |
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 |
C | N/A | ... | 0.10 | ... | -3.21 | 0.06 | 5.22 | C |
Na | N/A | ... | -0.10 | ... | -3.45 | -0.18 | 2.79 | Na |
Mg | N/A | ... | 0.40 | ... | -3.06 | 0.21 | 4.54 | Mg |
Ca | N/A | ... | 0.35 | ... | -3.07 | 0.20 | 3.27 | Ca |
Fe I | N/A | -3.44 | ... | ... | -3.27 | ... | 4.23 | Fe I |
Fe II | N/A | -3.45 | ... | ... | -3.28 | ... | 4.22 | Fe II |
Ni | N/A | ... | 0.83 | ... | -2.58 | 0.69 | 3.64 | Ni |
Sr | N/A | ... | -0.86 | ... | -4.27 | -1.00 | -1.40 | Sr |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FRUTTI | 22000 | N/A | N/A | N/A |
First stars IX - Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 |
C | N/A | -3.15+-0.08 | ... | ... | -3.06+-0.08 | 0.43+-0.08 | 5.37+-0.08 | C |
N | N/A | -3.22+-0.12 | ... | ... | -3.13+-0.12 | 0.36+-0.12 | 4.70+-0.12 | N |
Fe | N/A | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Isotopic Ratio
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 47000 | 130 | N/A | N/A |
NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 | -3.78 | -0.29 | 2.47 | -3.77 | -0.28 | 2.47 | Na |
Fe | N/A | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 43000 | 200 | N/A | N/A |
NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 |
Al | N/A | -3.73 | -0.24 | 2.74 | -3.71 | -0.22 | 2.74 | Al |
Fe | N/A | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 47000 | 120 | N/A | N/A |
Evolution of the barium abundance in the early Galaxy from a NLTE analysis of the Ba lines in a homogeneous sample of EMP stars
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Ba | 1 | ... | ... | -2.65 | -4.83 | -1.34 | -2.65 | Ba |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 45000 | 130 | N/A | N/A |
Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Milky Way
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 | N/A | ... | ... | 4.29 | -3.31 | 0.18 | 4.29 | Mg |
K | N/A | ... | ... | 2.20 | -2.83 | 0.66 | 2.20 | K |
Fe | N/A | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | VLT | 45000 | 120 | N/A | N/A |
First stars. XIV. Sulfur abundances in extremely metal-poor stars
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 |
S I | 2 | ... | ... | 4.25+-0.20 | -2.87+-0.20 | 0.62+-0.20 | 4.25+-0.20 | S I |
Fe | N/A | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 43000 | 180 | N/A | N/A |
First stars. VIII. Enrichment of the neutron-capture elements in the early Galaxy
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Sr | 2 | ... | -0.95 | ... | -4.39 | -0.90 | -1.52 | Sr |
Y | 1 | ... | -0.83 | ... | -4.29 | -0.80 | -2.08 | Y |
Zr | 1 | ... | -0.49 | ... | -3.96 | -0.47 | -1.38 | Zr |
Ba | 2 | ... | -1.29 | ... | -4.83 | -1.34 | -2.65 | Ba |
La | N/A | ... | <-0.18 | ... | <-3.60 | <-0.11 | <-2.50 | La |
Ce | N/A | ... | <+0.41 | ... | <-3.08 | <0.41 | <-1.50 | Ce |
Pr | N/A | ... | <+0.23 | ... | <-3.27 | <0.22 | <-2.55 | Pr |
Nd | N/A | ... | <-0.11 | ... | <-3.52 | <-0.03 | <-2.10 | Nd |
Sm | N/A | ... | <+0.88 | ... | <-2.56 | <0.93 | <-1.60 | Sm |
Eu | N/A | ... | <-0.02 | ... | <-3.52 | <-0.03 | <-3.00 | Eu |
Gd | 2 | ... | +1.12 | ... | -2.32 | 1.17 | -1.25 | Gd |
Dy | N/A | ... | <-0.35 | ... | <-3.80 | <-0.31 | <-2.70 | Dy |
Ho | N/A | ... | <+0.83 | ... | <-2.87 | <0.62 | <-2.40 | Ho |
Er | N/A | ... | <+0.56 | ... | <-2.92 | <0.57 | <-2.00 | Er |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 47000 | >50 | N/A | N/A |
NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 1.9 |
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 |
Ca | N/A | -3.09 | 0.40 | ... | -3.07 | 0.42 | 3.27 | Ca |
Fe | N/A | -3.49 | ... | ... | -3.49 | ... | 4.01 | Fe |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 45000 | 150 | N/A | N/A |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 4540+-34 | log g : 0.6+-0.14 | vturb : 1.65+-0.06 |
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 | 1 | ... | ... | 0.52 | -2.74 | 1.18 | 0.52 | Li I |
CH | 1 | ... | 0.23+-0.25 | 4.81 | -3.62 | 0.30+-0.25 | 4.81 | CH |
NH | 1 | ... | 0.25+-0.36 | 4.23 | -3.60 | 0.32+-0.36 | 4.23 | NH |
O I | 2 | ... | <1.51 | <6.28 | <-2.41 | <1.51 | <6.28 | O I |
Na I | 1 | ... | -0.10+-0.20 | 2.22 | -4.02 | -0.10+-0.20 | 2.22 | Na I |
Mg I | 8 | ... | 0.44+-0.16 | 4.12 | -3.48 | 0.44+-0.16 | 4.12 | Mg I |
Al I | 1 | ... | -0.80+-0.23 | 1.73 | -4.72 | -0.80+-0.23 | 1.73 | Al I |
Si I | 1 | ... | 0.84+-0.31 | 4.43 | -3.08 | 0.84+-0.31 | 4.43 | Si I |
Ca I | 12 | ... | 0.38+-0.18 | 2.80 | -3.54 | 0.38+-0.18 | 2.80 | Ca I |
Sc II | 4 | ... | -0.19+-0.15 | -0.88 | -4.03 | -0.11+-0.15 | -0.88 | Sc II |
Ti I | 7 | ... | 0.02+-0.16 | 1.05 | -3.90 | 0.02+-0.16 | 1.05 | Ti I |
Ti II | 19 | ... | -0.05+-0.15 | 1.05 | -3.90 | 0.02+-0.15 | 1.05 | Ti II |
V I | 1 | ... | <0.19 | <0.20 | <-3.73 | <0.19 | <0.20 | V I |
V II | 1 | ... | <0.26 | <0.34 | <-3.59 | <0.33 | <0.34 | V II |
Cr I | 6 | ... | -0.23+-0.15 | 1.49 | -4.15 | -0.23+-0.15 | 1.49 | Cr I |
Mn I | 3 | ... | -0.54+-0.17 | 0.98 | -4.45 | -0.53+-0.17 | 0.98 | Mn I |
Mn II | 3 | ... | -0.38+-0.21 | 1.21 | -4.22 | -0.30+-0.21 | 1.21 | Mn II |
Fe I | 105 | -3.92+-0.15 | ... | 3.58 | -3.92+-0.15 | ... | 3.58 | Fe I |
Fe II | 8 | -3.85+-0.16 | ... | 3.65 | -3.85+-0.16 | ... | 3.65 | Fe II |
Co I | 7 | ... | 0.05+-0.20 | 1.12 | -3.87 | 0.05+-0.20 | 1.12 | Co I |
Ni I | 5 | ... | 0.03+-0.20 | 2.34 | -3.88 | 0.04+-0.20 | 2.34 | Ni I |
Zn I | 2 | ... | 0.36+-0.21 | 1.00 | -3.56 | 0.36+-0.21 | 1.00 | Zn I |
Rb I | 1 | ... | <3.09 | <1.69 | <-0.67 | <3.25 | <1.69 | Rb I |
Sr II | 2 | ... | -0.96+-0.19 | -1.94 | -4.81 | -0.89+-0.19 | -1.94 | Sr II |
Y II | 5 | ... | <-0.93 | <-2.57 | <-4.78 | <-0.86 | <-2.57 | Y II |
Zr II | 2 | ... | <0.00 | <-1.27 | <-3.85 | <0.07 | <-1.27 | Zr II |
Nb II | 1 | ... | <2.21 | <-0.18 | <-1.64 | <2.28 | <-0.18 | Nb II |
Mo I | 1 | ... | <1.20 | <-0.84 | <-2.72 | <1.20 | <-0.84 | Mo I |
Tc I | 1 | ... | ... | <-0.36 | <-0.36 | <3.56 | <-0.36 | Tc I |
Ba II | 1 | ... | -1.59+-0.15 | -3.26 | -5.44 | -1.52+-0.15 | -3.26 | Ba II |
Ce II | 5 | ... | <0.09 | <-2.18 | <-3.76 | <0.16 | <-2.18 | Ce II |
Pr II | 1 | ... | <0.97 | <-2.16 | <-2.88 | <1.04 | <-2.16 | Pr II |
Nd II | 4 | ... | <0.08 | <-2.35 | <-3.77 | <0.15 | <-2.35 | Nd II |
Sm II | 2 | ... | <0.72 | <-2.17 | <-3.13 | <0.79 | <-2.17 | Sm II |
Eu II | 1 | ... | <0.25 | <-3.08 | <-3.60 | <0.32 | <-3.08 | Eu II |
Gd II | 3 | ... | <1.17 | <-1.61 | <-2.68 | <1.24 | <-1.61 | Gd II |
Tb II | 3 | ... | <0.92 | <-2.63 | <-2.95 | <0.97 | <-2.63 | Tb II |
Dy II | 3 | ... | <0.29 | <-2.46 | <-3.56 | <0.36 | <-2.46 | Dy II |
Ho II | 1 | ... | <0.92 | <-2.45 | <-2.92 | <1.00 | <-2.45 | Ho II |
Er II | 2 | ... | <0.71 | <-2.22 | <-3.14 | <0.78 | <-2.22 | Er II |
Tm II | 2 | ... | <1.05 | <-2.70 | <-2.82 | <1.10 | <-2.70 | Tm II |
Yb II | 1 | ... | <-0.38 | <-3.31 | <-4.23 | <-0.31 | <-3.31 | Yb II |
Hf II | 2 | ... | <1.46 | <-1.54 | <-2.25 | <1.67 | <-1.54 | Hf II |
Pb I | 1 | ... | <2.09 | <0.21 | <-1.83 | <2.09 | <0.21 | Pb I |
Th II | 3 | ... | <1.22 | <-2.57 | <-2.63 | <1.29 | <-2.57 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | -20.4 |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-09-26-08:13 | 2453274.847 | MIKELCO | 41000 | 85-150 | 3000 | -20.4 |
Stellar Chemical Signatures and Hierarchical Galaxy Formation
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 | ... | -0.1 | ... | -3.45 | -0.01 | 2.79 | Na |
Mg | N/A | ... | 0.4 | ... | -3.06 | 0.38 | 4.54 | Mg |
Ca | N/A | ... | 0.35 | ... | -3.07 | 0.37 | 3.27 | Ca |
Ti | N/A | ... | 0.34 | ... | -3.03 | 0.41 | 1.92 | Ti |
Fe | N/A | -3.44 | ... | ... | -3.44 | ... | 4.06 | Fe |
Ni | N/A | ... | 0.83 | ... | -2.58 | 0.86 | 3.64 | Ni |
Position
Right Ascension : 02 41 42.38 | Declination : -13 28 10.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log