CS22953-003
taken from 17 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)/
/I.U.Roederer et al.(2014)/
/T.Masseron et al.(2010)/
/F.Spite et al.(2018)/
/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 : 5100 | log g : 2.3 | 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 |
CH | N/A | -2.52 | 0.32 | 6.00 | -2.43 | 0.42 | 6.00 | CH |
[O I] | N/A | -2.09 | 0.75 | 6.68 | -2.01 | 0.84 | 6.68 | [O I] |
Na I | 2 | -2.69 | 0.15 | 3.64 | -2.60 | 0.25 | 3.64 | Na I |
Mg I | 7 | -2.71+-0.09 | 0.13+-0.09 | 4.87+-0.09 | -2.73+-0.09 | 0.12+-0.09 | 4.87+-0.09 | Mg I |
Al I | 2 | -3.82 | -0.99 | 2.65 | -3.80 | -0.95 | 2.65 | Al I |
Si I | 1 | -2.59 | 0.25 | 4.96 | -2.55 | 0.30 | 4.96 | Si I |
K I | 1 | -2.63 | 0.31 | 2.59 | -2.44 | 0.41 | 2.59 | K I |
Ca I | 17 | -2.62+-0.14 | 0.22+-0.14 | 3.74+-0.14 | -2.60+-0.14 | 0.25+-0.14 | 3.74+-0.14 | Ca I |
Sc II | 7 | -2.85+-0.08 | -0.02+-0.08 | 0.32+-0.08 | -2.83+-0.08 | 0.02+-0.08 | 0.32+-0.08 | Sc II |
Ti I | 14 | -2.69+-0.09 | 0.15+-0.09 | 2.33+-0.09 | -2.62+-0.09 | 0.23+-0.09 | 2.33+-0.09 | Ti I |
Ti II | 29 | -2.73+-0.10 | 0.11+-0.10 | 2.29+-0.10 | -2.66+-0.10 | 0.19+-0.10 | 2.29+-0.10 | Ti II |
Cr I | 7 | -3.24+-0.10 | -0.41+-0.10 | 2.43+-0.10 | -3.21+-0.10 | -0.36+-0.10 | 2.43+-0.10 | Cr I |
Mn I | 3 | -3.20+-0.05 | -0.37+-0.05 | 2.19+-0.05 | -3.24+-0.05 | -0.39+-0.05 | 2.19+-0.05 | Mn I |
Fe I | 148 | -2.85+-0.15 | -0.01+-0.15 | 4.65+-0.15 | -2.85+-0.15 | -0.01+-0.15 | 4.65+-0.15 | Fe I |
Fe II | 17 | -2.82+-0.11 | 0.01+-0.11 | 4.68+-0.11 | -2.82+-0.11 | 0.01+-0.11 | 4.68+-0.11 | Fe II |
Co I | 4 | -2.67+-0.10 | 0.17+-0.10 | 2.25+-0.10 | -2.74+-0.10 | 0.11+-0.10 | 2.25+-0.10 | Co I |
Ni I | 3 | -2.92+-0.05 | -0.09+-0.05 | 3.33+-0.05 | -2.89+-0.05 | -0.04+-0.05 | 3.33+-0.05 | Ni I |
Zn I | 1 | -2.69 | 0.15 | 1.91 | -2.65 | 0.20 | 1.91 | Zn I |
Binary Parameters
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-09 | N/A | VLT | 47000 | 140 | 13500 | 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 : 5100 | log g : 2.3 | 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 |
Li I | N/A | ... | ... | 0.80+-0.04 | -2.46+-0.04 | 0.38+-0.04 | 0.80+-0.04 | Li I |
C | N/A | -2.54+-0.03 | ... | ... | -2.45+-0.03 | 0.39+-0.03 | 5.98+-0.03 | C |
N | N/A | -2.72 | ... | ... | -2.63 | 0.21 | 5.20 | N |
[O I] | N/A | -2.09 | ... | ... | -2.04 | 0.80 | 6.65 | [O I] |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 4960 | log g : 1.70+-0.30 | vturb : 1.95+-0.10 |
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 | ... | 0.36 | ... | -2.32 | 0.32 | 6.11 | C |
Na | N/A | ... | -0.23 | ... | -2.95 | -0.31 | 3.29 | Na |
Mg | N/A | ... | 0.27 | ... | -2.56 | 0.08 | 5.04 | Mg |
Ca | N/A | ... | 0.31 | ... | -2.48 | 0.16 | 3.86 | Ca |
Fe I | N/A | -2.81 | ... | ... | -2.64 | ... | 4.86 | Fe I |
Fe II | N/A | -2.83 | ... | ... | -2.66 | ... | 4.84 | Fe II |
Ni | N/A | ... | 0.47 | ... | -2.31 | 0.33 | 3.91 | Ni |
Sr | N/A | ... | 0.31 | ... | -2.47 | 0.17 | 0.40 | Sr |
Ba | N/A | ... | 0.83 | ... | -2.03 | 0.61 | 0.15 | Ba |
Eu | N/A | ... | 0.72 | ... | -2.10 | 0.54 | -1.58 | Eu |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 |
C | N/A | -2.52+-0.03 | ... | ... | -2.43+-0.03 | 0.41+-0.03 | 6.00+-0.03 | C |
N | N/A | -2.72+-0.10 | ... | ... | -2.63+-0.10 | 0.21+-0.10 | 5.20+-0.10 | N |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Isotopic Ratio
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 | -3.05 | -0.21 | 3.20 | -3.04 | -0.20 | 3.20 | Na |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 |
Al | N/A | -3.02 | -0.18 | 3.45 | -3.00 | -0.16 | 3.45 | Al |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Ba | 3 | ... | ... | -0.22 | -2.40 | 0.44 | -0.22 | Ba |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 |
Mg | N/A | ... | ... | 5.03 | -2.57 | 0.27 | 5.03 | Mg |
K | N/A | ... | ... | 2.60 | -2.43 | 0.41 | 2.60 | K |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 |
S I | 2 | ... | ... | 4.72+-0.10 | -2.40+-0.10 | 0.44+-0.10 | 4.72+-0.10 | S I |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Sr | 3 | ... | +0.22 | ... | -2.57 | 0.27 | 0.30 | Sr |
Y | 10 | ... | +0.14 | ... | -2.67 | 0.17 | -0.46 | Y |
Zr | 11 | ... | +0.36 | ... | -2.46 | 0.38 | 0.12 | Zr |
Ba | 5 | ... | +0.49 | ... | -2.40 | 0.44 | -0.22 | Ba |
La | 7 | ... | +0.66 | ... | -2.11 | 0.73 | -1.01 | La |
Ce | 2 | ... | +0.66 | ... | -2.18 | 0.66 | -0.60 | Ce |
Pr | 1 | ... | +0.68 | ... | -2.17 | 0.67 | -1.45 | Pr |
Nd | 2 | ... | +0.72 | ... | -2.04 | 0.80 | -0.62 | Nd |
Sm | 2 | ... | +0.34 | ... | -2.45 | 0.39 | -1.49 | Sm |
Eu | 1 | ... | +1.05 | ... | -1.80 | 1.04 | -1.28 | Eu |
Gd | 4 | ... | +1.01 | ... | -1.78 | 1.06 | -0.71 | Gd |
Dy | 12 | ... | +1.04 | ... | -1.76 | 1.08 | -0.66 | Dy |
Ho | 1 | ... | +1.18 | ... | -1.87 | 0.97 | -1.40 | Ho |
Er | 2 | ... | +1.06 | ... | -1.77 | 1.07 | -0.85 | Er |
Yb | 1 | ... | +1.02 | ... | -1.66 | 1.18 | -0.74 | Yb |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 5100 | log g : 2.3 | 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 |
Ca | N/A | -2.47 | 0.37 | ... | -2.45 | 0.39 | 3.89 | Ca |
Fe | N/A | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 : 4860+-37 | log g : 1.65+-0.17 | vturb : 1.45+-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 | ... | ... | 0.64 | -2.62 | 0.51 | 0.64 | Li I |
CH | 1 | ... | 0.10+-0.25 | 5.53 | -2.90 | 0.23+-0.25 | 5.53 | CH |
NH | 1 | ... | -0.30+-0.36 | 4.53 | -3.30 | -0.17+-0.36 | 4.53 | NH |
O I | 4 | ... | <1.17 | <6.73 | <-1.96 | <1.17 | <6.73 | O I |
Na I | 1 | ... | -0.03+-0.29 | 3.08 | -3.16 | -0.03+-0.29 | 3.08 | Na I |
Mg I | 9 | ... | 0.39+-0.16 | 4.86 | -2.74 | 0.39+-0.16 | 4.86 | Mg I |
Al I | 1 | ... | -0.80+-0.29 | 2.52 | -3.93 | -0.80+-0.29 | 2.52 | Al I |
Si I | 1 | ... | 0.94+-0.23 | 5.32 | -2.19 | 0.94+-0.23 | 5.32 | Si I |
Ca I | 11 | ... | 0.33+-0.17 | 3.54 | -2.80 | 0.33+-0.17 | 3.54 | Ca I |
Sc II | 5 | ... | -0.23+-0.15 | -0.07 | -3.22 | -0.09+-0.15 | -0.07 | Sc II |
Ti I | 11 | ... | 0.07+-0.15 | 1.89 | -3.06 | 0.07+-0.15 | 1.89 | Ti I |
Ti II | 33 | ... | 0.04+-0.15 | 2.00 | -2.95 | 0.18+-0.15 | 2.00 | Ti II |
V I | 1 | ... | -0.24+-0.19 | 0.56 | -3.37 | -0.24+-0.19 | 0.56 | V I |
V II | 2 | ... | -0.03+-0.25 | 0.90 | -3.03 | 0.10+-0.25 | 0.90 | V II |
Cr I | 5 | ... | -0.25+-0.15 | 2.26 | -3.38 | -0.25+-0.15 | 2.26 | Cr I |
Cr II | 2 | ... | -0.12+-0.18 | 2.52 | -3.12 | 0.01+-0.18 | 2.52 | Cr II |
Mn I | 2 | ... | -0.40+-0.15 | 1.90 | -3.53 | -0.40+-0.15 | 1.90 | Mn I |
Mn II | 4 | ... | -0.48+-0.21 | 1.95 | -3.48 | -0.35+-0.21 | 1.95 | Mn II |
Fe I | 105 | -3.13+-0.14 | ... | 4.37 | -3.13+-0.14 | ... | 4.37 | Fe I |
Fe II | 11 | -3.00+-0.15 | ... | 4.50 | -3.00+-0.15 | ... | 4.50 | Fe II |
Co I | 6 | ... | -0.13+-0.21 | 1.73 | -3.26 | -0.13+-0.21 | 1.73 | Co I |
Ni I | 11 | ... | 0.18+-0.21 | 3.27 | -2.95 | 0.18+-0.21 | 3.27 | Ni I |
Zn I | 2 | ... | 0.37+-0.15 | 1.80 | -2.76 | 0.37+-0.15 | 1.80 | Zn I |
Rb I | 1 | ... | <2.62 | <2.01 | <-0.35 | <2.78 | <2.01 | Rb I |
Sr II | 2 | ... | 0.32+-0.24 | 0.19 | -2.68 | 0.45+-0.24 | 0.19 | Sr II |
Y II | 4 | ... | -0.16+-0.16 | -0.95 | -3.16 | -0.03+-0.16 | -0.95 | Y II |
Zr II | 3 | ... | 0.24+-0.16 | -0.18 | -2.76 | 0.37+-0.16 | -0.18 | Zr II |
Nb II | 1 | ... | <1.77 | <0.23 | <-1.23 | <1.90 | <0.23 | Nb II |
Mo I | 1 | ... | <1.00 | <-0.25 | <-2.13 | <1.00 | <-0.25 | Mo I |
Tc I | 1 | ... | ... | <0.18 | <0.18 | <3.31 | <0.18 | Tc I |
Sn I | 1 | ... | <2.11 | <1.05 | <-1.02 | <2.11 | <1.05 | Sn I |
Ba II | 4 | ... | 0.29+-0.15 | -0.53 | -2.71 | 0.42+-0.15 | -0.53 | Ba II |
La II | 4 | ... | 0.43+-0.16 | -1.47 | -2.57 | 0.56+-0.16 | -1.47 | La II |
Ce II | 2 | ... | 0.40+-0.22 | -1.01 | -2.59 | 0.54+-0.22 | -1.01 | Ce II |
Pr II | 2 | ... | 0.57+-0.19 | -1.70 | -2.42 | 0.71+-0.19 | -1.70 | Pr II |
Nd II | 5 | ... | 0.57+-0.17 | -1.01 | -2.43 | 0.70+-0.17 | -1.01 | Nd II |
Sm II | 2 | ... | 0.67+-0.18 | -1.37 | -2.33 | 0.80+-0.18 | -1.37 | Sm II |
Eu II | 4 | ... | 0.79+-0.15 | -1.69 | -2.21 | 0.92+-0.15 | -1.69 | Eu II |
Gd II | 2 | ... | 0.98+-0.21 | -0.94 | -2.01 | 1.12+-0.21 | -0.94 | Gd II |
Tb II | 2 | ... | <1.49 | <-1.21 | <-1.53 | <1.60 | <-1.21 | Tb II |
Dy II | 3 | ... | 1.02+-0.17 | -0.87 | -1.97 | 1.16+-0.17 | -0.87 | Dy II |
Ho II | 2 | ... | 0.84+-0.21 | -1.67 | -2.14 | 0.99+-0.21 | -1.67 | Ho II |
Er II | 3 | ... | 0.84+-0.18 | -1.23 | -2.15 | 0.98+-0.18 | -1.23 | Er II |
Tm II | 1 | ... | 0.93+-0.24 | -1.97 | -2.09 | 1.04+-0.24 | -1.97 | Tm II |
Yb II | 1 | ... | 0.63+-0.20 | -1.45 | -2.37 | 0.76+-0.20 | -1.45 | Yb II |
Hf II | 2 | ... | <1.36 | <-0.79 | <-1.50 | <1.63 | <-0.79 | Hf II |
Ir I | 1 | ... | 1.28+-0.41 | -0.47 | -1.85 | 1.28+-0.41 | -0.47 | Ir I |
Pb I | 1 | ... | <1.50 | <0.41 | <-1.63 | <1.50 | <0.41 | Pb I |
Th II | 1 | ... | 1.02+-0.22 | -1.92 | -1.98 | 1.15+-0.22 | -1.92 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | 208.3 |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-08-03-09:46 | 2453950.91 | MIKELCO | 41000 | 65-100 | 2000 | 208.3 |
Nine new metal-poor stars on the subgiant and red horizontal branches with high levels of r-process enhancement
Stellar Parameters
Teff : 4860+-151 | log g : 1.65+-0.40 | vturb : 1.45+-0.41 |
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 | -3.00+-0.07 | ... | ... | -3.00+-0.07 | ... | 4.50+-0.07 | Fe |
Sr | N/A | ... | +0.32+-0.24 | ... | -2.68+-0.24 | 0.32+-0.24 | 0.19+-0.24 | Sr |
Ba | N/A | ... | +0.29+-0.15 | ... | -2.71+-0.15 | 0.29+-0.15 | -0.53+-0.15 | Ba |
Eu | N/A | ... | +0.79+-0.15 | ... | -2.21+-0.15 | 0.79+-0.15 | -1.69+-0.15 | Eu |
Yb | N/A | ... | +0.63+-0.20 | ... | -2.37+-0.20 | 0.63+-0.20 | -1.45+-0.20 | Yb |
Binary Parameters
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-08-03 | 2453950.910 | MIKELCO | 41000 | 65-100 | 2000 | +208.3 |
A holistic approach to carbon-enhanced metal-poor stars
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 |
C | N/A | ... | 0.39+-0.1 | ... | -2.53+-0.1 | 0.40+-0.1 | 5.90+-0.1 | C |
N | N/A | ... | 0.7+-0.1 | ... | -2.23+-0.1 | 0.70+-0.1 | 5.60+-0.1 | N |
O | N/A | ... | <1.22 | ... | <-1.69 | <1.24 | <7.00 | O |
Mg | N/A | ... | 0.46+-0.19 | ... | -2.49+-0.19 | 0.44+-0.19 | 5.11+-0.19 | Mg |
Fe | N/A | -2.88+-0.16 | ... | ... | -2.93+-0.16 | ... | 4.57+-0.16 | Fe |
Ba | N/A | ... | 0.31+-0.1 | ... | -2.58+-0.1 | 0.35+-0.1 | -0.40+-0.1 | Ba |
La | N/A | ... | 0.55+-0.1 | ... | -2.30+-0.1 | 0.63+-0.1 | -1.20+-0.1 | La |
Ce | N/A | ... | 2.06+-0.18 | ... | -0.82+-0.18 | 2.11+-0.18 | 0.76+-0.18 | Ce |
Pb | N/A | ... | 1.85+-0.2 | ... | -1.05+-0.2 | 1.88+-0.2 | 0.99+-0.2 | Pb |
Isotopic Ratio
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | 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 | R=40000 | N/A | N/A | N/A |
Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars
Stellar Parameters
Teff : 5100+-100 | log g : 2.3+-0.2 | vturb : 1.7+-2 |
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 | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe |
Sr | N/A | ... | 0.24+-0.2 | 0.30+-0.2 | -2.57+-0.2 | 0.27+-0.2 | 0.30+-0.2 | Sr |
Y | N/A | ... | 0.18+-0.2 | -0.46+-0.2 | -2.67+-0.2 | 0.17+-0.2 | -0.46+-0.2 | Y |
Zr | N/A | ... | 0.39+-0.2 | 0.12+-0.2 | -2.46+-0.2 | 0.38+-0.2 | 0.12+-0.2 | Zr |
Mo | N/A | ... | 0.40+-0.25 | -0.50+-0.25 | -2.38+-0.25 | 0.46+-0.25 | -0.50+-0.25 | Mo |
Ru | N/A | ... | 0.81+-0.25 | -0.25+-0.25 | -2.00+-0.25 | 0.84+-0.25 | -0.25+-0.25 | Ru |
Pd | N/A | ... | 0.47+-0.25 | -0.70+-0.25 | -2.27+-0.25 | 0.57+-0.25 | -0.70+-0.25 | Pd |
Ba | N/A | ... | 0.44 | -0.22 | -2.40 | 0.44 | -0.22 | Ba |
Eu | N/A | ... | 1.03 | -1.28 | -1.80 | 1.04 | -1.28 | Eu |
Position
Right Ascension : 01 02 15.87 | Declination : -61 43 45.83 | 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 | 150 | N/A | N/A |
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 | ... | -0.23 | ... | -2.96 | -0.14 | 3.28 | Na |
Mg | N/A | ... | 0.27 | ... | -2.57 | 0.25 | 5.03 | Mg |
Ca | N/A | ... | 0.31 | ... | -2.49 | 0.33 | 3.85 | Ca |
Ti | N/A | ... | 0.13 | ... | -2.62 | 0.20 | 2.33 | Ti |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Ni | N/A | ... | 0.47 | ... | -2.32 | 0.50 | 3.90 | Ni |
Y | N/A | ... | 0.22 | ... | -2.57 | 0.25 | -0.36 | Y |
Eu | N/A | ... | 0.72 | ... | -2.11 | 0.71 | -1.59 | Eu |
Position
Right Ascension : 01 02 15.86 | Declination : -61 43 45.8 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log