CS22949-037
HE2323-0256 in J.G.Cohen+,ApJ, 672, 320, 2008
taken from 18 paper(s):
/E.Depagne et al.(2002)/
/J.E.Norris et al.(2001)/
/R.Cayrel et al.(2004)/
/M.Spite et al.(2005)/
/J.E.Norris et al.(2002)/
/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.(2009)/
/S.M.Andrievsky et al.(2010)/
/M.Spite et al.(2011)/
/M.Spite et al.(2012)/
/I.U.Roederer et al.(2014)/
/I.U.Roederer et al.(2014)/
/F.Spite et al.(2018)/
/A.Arentsen et al.(2019)/
/K.A.Venn et al.(2004)/
First Stars II. Elemental abundances in the extremely metal-poor star CS 22949–037 A diagnostic of early massive supernovae
Stellar Parameters
Teff : 4900 | log g : 1.5 | vturb : 1.8 |
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 | -2.8 | 1.17 | 5.72 | -2.71 | 1.28 | 5.72 | C |
CN | N/A | -1.4 | 2.57 | 6.52 | -1.31 | 2.68 | 6.52 | CN |
O I | 1 | -1.99 | 1.98 | 6.84 | -1.85 | 2.14 | 6.84 | O I |
Na I | 2 | -1.88+-0.03 | 2.09+-0.03 | 3.8+-0.03 | -2.44+-0.03 | 1.55+-0.03 | 3.8+-0.03 | Na I |
Mg I | 4 | -2.41+-0.19 | 1.58+-0.19 | 5.17+-0.19 | -2.43+-0.19 | 1.56+-0.19 | 5.17+-0.19 | Mg I |
Al I | 2 | -4.13+-0.03 | -0.16+-0.03 | 2.34+-0.03 | -4.11+-0.03 | -0.12+-0.03 | 2.34+-0.03 | Al I |
Si I | 2 | -3.25 | 0.72 | 4.05 | -3.46 | 0.53 | 4.05 | Si I |
S I | 1 | -2.12 | +1.78 | 5.09 | -2.03 | 1.96 | 5.09 | S I |
K I | 2 | -4.06 | -0.09 | 0.89 | -4.14 | -0.15 | 0.89 | K I |
Ca I | 10 | -3.63+-0.17 | 0.35+-0.17 | 2.73+-0.17 | -3.61+-0.17 | 0.38+-0.17 | 2.73+-0.17 | Ca I |
Sc II | 5 | -3.87+-0.14 | 0.1+-0.14 | -0.7+-0.14 | -3.85+-0.14 | 0.14+-0.14 | -0.7+-0.14 | Sc II |
Ti I | 8 | -3.62+-0.09 | 0.35+-0.09 | 1.4+-0.09 | -3.55+-0.09 | 0.44+-0.09 | 1.4+-0.09 | Ti I |
Ti II | 21 | -3.61+-0.15 | 0.36+-0.15 | 1.41+-0.15 | -3.54+-0.15 | 0.45+-0.15 | 1.41+-0.15 | Ti II |
Cr I | 5 | -4.38+-0.1 | -0.41+-0.1 | 1.29+-0.1 | -4.35+-0.1 | -0.36+-0.1 | 1.29+-0.1 | Cr I |
Mn I | 2 | -4.78+-0.01 | -0.81+-0.01 | 0.61+-0.01 | -4.82+-0.01 | -0.83+-0.01 | 0.61+-0.01 | Mn I |
Fe I | 64 | -3.99+-0.11 | ... | 3.51+-0.11 | -3.99+-0.11 | ... | 3.51+-0.11 | Fe I |
Fe II | 6 | -3.94+-0.11 | ... | 3.56+-0.11 | -3.94+-0.11 | ... | 3.56+-0.11 | Fe II |
Co I | 4 | -3.64+-0.07 | 0.33+-0.07 | 1.28+-0.07 | -3.71+-0.07 | 0.28+-0.07 | 1.28+-0.07 | Co I |
Ni I | 3 | -4.06+-0.02 | -0.07+-0.02 | 2.19+-0.02 | -4.03+-0.02 | -0.04+-0.02 | 2.19+-0.02 | Ni I |
Zn I | 1 | -3.41 | 0.7 | 1.29 | -3.27 | 0.72 | 1.29 | Zn I |
Sr II | 2 | -3.64+-0.06 | 0.33+-0.06 | -0.72+-0.06 | -3.59+-0.06 | 0.40+-0.06 | -0.72+-0.06 | Sr II |
Y II | 3 | -4.04+-0.11 | -0.07+-0.11 | -1.8+-0.11 | -4.01+-0.11 | -0.02+-0.11 | -1.8+-0.11 | Y II |
Ba II | 4 | -4.55+-0.1 | -0.58+-0.1 | -2.42+-0.1 | -4.60+-0.1 | -0.61+-0.1 | -2.42+-0.1 | Ba II |
Sm II | 1 | -2.83 | +1.14 | -1.82 | -2.78 | 1.21 | -1.82 | Sm II |
Eu II | 1 | -3.93 | +0.04 | -3.42 | -3.94 | 0.05 | -3.42 | Eu II |
Binary Parameters
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-08-08-04:54:00 | N/A | VLT | 45000 | 110-170 | 3600 | -125.68+-0.2 |
2000-08-08-05:57:00 | N/A | VLT | 45000 | 110-170 | 3600 | |
2000-08-09-04:01:00 | N/A | VLT | 45000 | 110-170 | 3600 | |
2000-08-09-05:04:00 | N/A | VLT | 45000 | 110-170 | 3600 | -125.64+-0.2 |
2000-08-11-04:27:00 | N/A | VLT | 45000 | 110-170 | 3600 | -125.60+-0.2 |
2000-08-11-05:36:00 | N/A | VLT | 45000 | 110-170 | 3600 | |
2001-09-06-05:06:00 | N/A | VLT | 45000 | 40-90 | 3600 | -125.62+-0.2 |
EXTREMELY METAL-POOR STARS. VIII. HIGH-RESOLUTION, HIGH SIGNAL-TO-NOISE RATIO ANALYSIS OF FIVE STARS WITH [Fe/H]<=-3.5
Stellar Parameters
Teff : 4900 | log g : 1.7 | vturb : 2.0 |
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 | ... | 1.05+-0.20 | ... | -2.50+-0.20 | 1.12+-0.20 | 5.93+-0.20 | CH |
CN | N/A | ... | 2.70+-0.40 | ... | -0.93+-0.40 | 2.69+-0.40 | 6.90+-0.40 | CN |
Mg I | 5 | ... | 1.22+-0.14 | ... | -2.59+-0.14 | 1.03+-0.14 | 5.01+-0.14 | Mg I |
Al I | 1 | ... | -0.43+-0.32 | ... | -4.20+-0.32 | -0.58+-0.32 | 2.25+-0.32 | Al I |
Si I | 2 | ... | 1.04+-0.30 | ... | -2.71+-0.30 | 0.91+-0.30 | 4.80+-0.30 | Si I |
Ca I | 3 | ... | 0.45+-0.21 | ... | -3.32+-0.21 | 0.30+-0.21 | 3.02+-0.21 | Ca I |
Sc II | 4 | ... | 0.13+-0.20 | ... | -3.72+-0.20 | -0.10+-0.20 | -0.57+-0.20 | Sc II |
Ti I | 1 | ... | <0.02+-0.04 | ... | <-3.73+-0.04 | <-0.11+-0.04 | <1.22+-0.04 | Ti I |
Ti II | 18 | ... | 0.35+-0.16 | ... | -3.40+-0.16 | 0.22+-0.16 | 1.55+-0.16 | Ti II |
V II | 1 | ... | <0.65+-0.19 | ... | <-3.07+-0.19 | <0.55+-0.19 | <0.86+-0.19 | V II |
Cr I | 3 | ... | -0.55+-0.17 | ... | -4.31+-0.17 | -0.69+-0.17 | 1.33+-0.17 | Cr I |
Mn I | 2 | ... | -0.92+-0.21 | ... | -4.75+-0.21 | -1.13+-0.21 | 0.68+-0.21 | Mn I |
Fe I | 61 | -3.79+-0.16 | ... | ... | -3.62+-0.16 | ... | 3.88+-0.16 | Fe I |
Fe II | 2 | -3.79+-0.29 | ... | ... | -3.62+-0.29 | ... | 3.88+-0.29 | Fe II |
Co I | 2 | ... | 0.58+-0.21 | ... | -3.28+-0.21 | 0.34+-0.21 | 1.71+-0.21 | Co I |
Ni I | 4 | ... | 0.06+-0.15 | ... | -3.70+-0.15 | -0.08+-0.15 | 2.52+-0.15 | Ni I |
Sr II | 2 | ... | 0.10+-0.23 | ... | -3.66+-0.23 | -0.04+-0.23 | -0.79+-0.23 | Sr II |
Y II | 2 | ... | 0.19+-0.25 | ... | -3.57+-0.25 | 0.05+-0.25 | -1.36+-0.25 | Y II |
Ba II | 1 | ... | -0.84+-0.32 | ... | -4.68+-0.32 | -1.06+-0.32 | -2.50+-0.32 | Ba II |
Eu II | 1 | ... | <0.93+-0.18 | ... | <-2.87+-0.18 | <0.75+-0.18 | <-2.35+-0.18 | Eu II |
Binary Parameters
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-09-05 | N/A | ANGLO | 42000 | N/A | N/A | -125.7+-1.19 |
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Stellar Parameters
Teff : 4900 | log g : 1.5 | vturb : 1.8 |
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 | -2.80 | 1.17 | 5.72 | -2.71 | 1.28 | 5.72 | CH |
CN | N/A | -1.40 | 2.57 | 6.52 | -1.31 | 2.68 | 6.52 | CN |
[O I] | N/A | -1.99 | 1.98 | 6.78 | -1.91 | 2.08 | 6.78 | [O I] |
Na I | 2 | -2.53 | 1.44 | 3.80 | -2.44 | 1.55 | 3.80 | Na I |
Mg I | 7 | -2.41+-0.19 | 1.56+-0.19 | 5.17+-0.19 | -2.43+-0.19 | 1.56+-0.19 | 5.17+-0.19 | Mg I |
Al I | 2 | -4.13 | -0.17 | 2.34 | -4.11 | -0.12 | 2.34 | Al I |
Si I | 1 | -3.20 | 0.77 | 4.35 | -3.16 | 0.83 | 4.35 | Si I |
K I | 2 | -3.74 | 0.23 | 1.38 | -3.65 | 0.34 | 1.38 | K I |
Ca I | 10 | -3.63+-0.17 | 0.34+-0.17 | 2.73+-0.17 | -3.61+-0.17 | 0.38+-0.17 | 2.73+-0.17 | Ca I |
Sc II | 5 | -3.87+-0.14 | 0.09+-0.14 | -0.70+-0.14 | -3.85+-0.14 | 0.14+-0.14 | -0.70+-0.14 | Sc II |
Ti I | 8 | -3.62+-0.09 | 0.35+-0.09 | 1.40+-0.09 | -3.55+-0.09 | 0.44+-0.09 | 1.40+-0.09 | Ti I |
Ti II | 21 | -3.61+-0.15 | 0.36+-0.15 | 1.41+-0.15 | -3.54+-0.15 | 0.45+-0.15 | 1.41+-0.15 | Ti II |
Cr I | 5 | -4.38+-0.10 | -0.42+-0.10 | 1.29+-0.10 | -4.35+-0.10 | -0.36+-0.10 | 1.29+-0.10 | Cr I |
Mn I | 2 | -4.43 | -0.47 | 0.96 | -4.47 | -0.48 | 0.96 | Mn I |
Fe I | 64 | -3.99+-0.11 | -0.03+-0.11 | 3.51+-0.11 | -3.99+-0.11 | -0.03+-0.11 | 3.51+-0.11 | Fe I |
Fe II | 6 | -3.94+-0.11 | 0.02+-0.11 | 3.56+-0.11 | -3.94+-0.11 | 0.02+-0.11 | 3.56+-0.11 | Fe II |
Co I | 4 | -3.64+-0.07 | 0.33+-0.07 | 1.28+-0.07 | -3.71+-0.07 | 0.28+-0.07 | 1.28+-0.07 | Co I |
Ni I | 3 | -4.06+-0.02 | -0.10+-0.02 | 2.19+-0.02 | -4.03+-0.02 | -0.04+-0.02 | 2.19+-0.02 | Ni I |
Zn I | 1 | -3.31 | 0.66 | 1.29 | -3.27 | 0.72 | 1.29 | Zn I |
Binary Parameters
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-08 | N/A | VLT | 47000 | 110 | 30000 | N/A |
2001-09 | N/A | VLT | N/A | N/A | N/A | 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 : 1.5 | vturb : 1.8 |
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 | ... | ... | <-0.30 | <-3.56 | <0.41 | <-0.30 | Li I |
C | N/A | -2.82+-0.10 | ... | ... | -2.73+-0.10 | 1.24+-0.10 | 5.70+-0.10 | C |
N | N/A | -1.82 | ... | ... | -1.73 | 2.24 | 6.10 | N |
[O I] | N/A | -1.99 | ... | ... | -1.94 | 2.03 | 6.75 | [O I] |
Fe | N/A | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 |
EXTREMELY METAL-POOR STARS. IX. CS 22949-037 AND THE ROLE OF HYPERNOVAE
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 | ... | 1.05 | ... | -2.62 | 1.17 | 5.81 | C |
CN | N/A | ... | 2.3+-0.4 | ... | -1.35+-0.4 | 2.44+-0.4 | 6.48+-0.4 | CN |
Fe | N/A | -3.79 | ... | ... | -3.79 | ... | 3.71 | Fe |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-08-24 | N/A | ANGLO | N/A | N/A | 300min | N/A |
2001-07-28 | N/A | SUBARUEEV | N/A | N/A | 165min | N/A |
A Spectroscopic Analysis of 33 of the Most Metal-Poor Stars.I.
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 : 4810 | log g : 2.10+-0.45 | vturb : 2.09+-0.17 |
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 | ... | 0.88 | ... | -2.98 | 0.84 | 5.45 | C |
Na | N/A | ... | 2.16 | ... | -1.74 | 2.08 | 4.50 | Na |
Mg | N/A | ... | 1.20 | ... | -2.81 | 1.01 | 4.79 | Mg |
Ca | N/A | ... | 0.90 | ... | -3.07 | 0.75 | 3.27 | Ca |
Fe I | N/A | -3.99 | ... | ... | -3.82 | ... | 3.68 | Fe I |
Fe II | N/A | -3.99 | ... | ... | -3.82 | ... | 3.68 | Fe II |
Sr | N/A | ... | 0.42 | ... | -3.54 | 0.28 | -0.67 | Sr |
Ba | N/A | ... | -0.16 | ... | -4.20 | -0.38 | -2.02 | Ba |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 : 1.5 | vturb : 1.8 |
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 | -2.72+-0.10 | ... | ... | -2.63+-0.10 | 1.34+-0.10 | 5.80+-0.10 | C |
N | N/A | -1.72+-0.30 | ... | ... | -1.63+-0.30 | 2.34+-0.30 | 6.20+-0.30 | N |
Fe | N/A | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Isotopic Ratio
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 : 1.5 | vturb : 1.8 |
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 | -2.40 | +1.57 | 3.85 | -2.39 | 1.58 | 3.85 | Na |
Fe | N/A | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 |
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 : 1.5 | vturb : 1.8 |
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 | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Ba | 1 | ... | ... | -2.42 | -4.60 | -0.63 | -2.42 | Ba |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 : 1.5 | vturb : 1.8 |
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 | ... | ... | 5.07 | -2.53 | 1.44 | 5.07 | Mg |
K | N/A | ... | ... | 1.50 | -3.53 | 0.44 | 1.50 | K |
Fe | N/A | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 : 1.5 | vturb : 1.8 |
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 | ... | ... | <3.9 | <-3.22 | <0.75 | <3.9 | S I |
Fe | N/A | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
Stellar Parameters
Teff : 4900 | log g : 1.5 | vturb : 1.8 |
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 | -3.35 | 0.61 | ... | -3.33 | 0.64 | 3.01 | Ca |
Fe | N/A | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | 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 |
Neutron-capture Nucleosynthesis in the First Stars
Stellar Parameters
Teff : 4630+-34 | log g : 0.95+-0.13 | vturb : 1.70+-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 | ... | ... | <0.13 | <-3.13 | <1.25 | <0.13 | Li I |
CH | 1 | ... | 0.99+-0.25 | 5.21+-0.25 | -3.22+-0.25 | 1.16+-0.25 | 5.21+-0.25 | CH |
NH | 1 | ... | 2.50+-0.36 | 6.12+-0.36 | -1.71+-0.36 | 2.67+-0.36 | 6.12+-0.36 | NH |
O I | 2 | ... | <2.39 | <6.70 | <-1.99 | <2.39 | <6.70 | O I |
Mg I | 7 | ... | 1.56+-0.15 | 4.78+-0.15 | -2.82+-0.15 | 1.56+-0.15 | 4.78+-0.15 | Mg I |
Al I | 1 | ... | 0.26+-0.29 | 2.33+-0.29 | -4.12+-0.29 | 0.26+-0.29 | 2.33+-0.29 | Al I |
Si I | 1 | ... | 1.52+-0.28 | 4.65+-0.28 | -2.86+-0.28 | 1.52+-0.28 | 4.65+-0.28 | Si I |
Ca I | 9 | ... | 0.67+-0.18 | 2.63+-0.18 | -3.71+-0.18 | 0.67+-0.18 | 2.63+-0.18 | Ca I |
Sc II | 5 | ... | -0.14+-0.16 | -1.20+-0.16 | -4.35+-0.16 | 0.03+-0.16 | -1.20+-0.16 | Sc II |
Ti I | 3 | ... | 0.28+-0.17 | 0.85+-0.17 | -4.10+-0.17 | 0.28+-0.17 | 0.85+-0.17 | Ti I |
Ti II | 14 | ... | 0.19+-0.15 | 0.94+-0.15 | -4.01+-0.15 | 0.37+-0.15 | 0.94+-0.15 | Ti II |
V II | 2 | ... | <0.46 | <0.19 | <-3.74 | <0.64 | <0.19 | V II |
Cr I | 4 | ... | -0.39+-0.15 | 0.87+-0.15 | -4.77+-0.15 | -0.39+-0.15 | 0.87+-0.15 | Cr I |
Mn I | 3 | ... | -0.64+-0.14 | 0.41+-0.14 | -5.02+-0.14 | -0.64+-0.14 | 0.41+-0.14 | Mn I |
Fe I | 58 | -4.38+-0.15 | ... | 3.12+-0.15 | -4.38+-0.15 | ... | 3.12+-0.15 | Fe I |
Fe II | 2 | -4.20+-0.16 | ... | 3.30+-0.16 | -4.20+-0.16 | ... | 3.30+-0.16 | Fe II |
Co I | 3 | ... | 0.19+-0.18 | 0.81+-0.18 | -4.18+-0.18 | 0.20+-0.18 | 0.81+-0.18 | Co I |
Ni I | 6 | ... | 0.10+-0.23 | 1.94+-0.23 | -4.28+-0.23 | 0.10+-0.23 | 1.94+-0.23 | Ni I |
Zn I | 2 | ... | <1.22 | <1.40 | <-3.16 | <1.22 | <1.40 | Zn I |
Rb I | 1 | ... | <3.51 | <1.65 | <-0.71 | <3.67 | <1.65 | Rb I |
Sr II | 2 | ... | 0.31+-0.25 | -1.02+-0.25 | -3.89+-0.25 | 0.49+-0.25 | -1.02+-0.25 | Sr II |
Y II | 2 | ... | -0.25+-0.19 | -2.25+-0.19 | -4.46+-0.19 | -0.08+-0.19 | -2.25+-0.19 | Y II |
Zr II | 2 | ... | 0.48+-0.19 | -1.15+-0.19 | -3.73+-0.19 | 0.65+-0.19 | -1.15+-0.19 | Zr II |
Nb II | 1 | ... | <2.64 | <-0.10 | <-1.56 | <2.82 | <-0.10 | Nb II |
Mo I | 1 | ... | <1.98 | <-0.52 | <-2.40 | <1.98 | <-0.52 | Mo I |
Sn I | 1 | ... | <3.21 | <0.90 | <-1.17 | <3.21 | <0.90 | Sn I |
Ba II | 2 | ... | -0.78+-0.16 | -2.80+-0.16 | -4.98+-0.16 | -0.60+-0.16 | -2.80+-0.16 | Ba II |
Ce II | 5 | ... | <0.74 | <-1.88 | <-3.46 | <0.92 | <-1.88 | Ce II |
Pr II | 4 | ... | <1.24 | <-2.24 | <-2.96 | <1.42 | <-2.24 | Pr II |
Nd II | 5 | ... | <0.65 | <-2.13 | <-3.55 | <0.83 | <-2.13 | Nd II |
Sm II | 2 | ... | <1.26 | <-1.98 | <-2.94 | <1.44 | <-1.98 | Sm II |
Eu II | 4 | ... | <0.51 | <-3.17 | <-3.69 | <0.69 | <-3.17 | Eu II |
Gd II | 1 | ... | <1.79 | <-1.34 | <-2.41 | <1.97 | <-1.34 | Gd II |
Tb II | 3 | ... | <1.48 | <-2.42 | <-2.74 | <1.64 | <-2.42 | Tb II |
Dy II | 3 | ... | <0.85 | <-2.25 | <-3.35 | <1.03 | <-2.25 | Dy II |
Ho II | 2 | ... | <1.36 | <-2.36 | <-2.83 | <1.55 | <-2.36 | Ho II |
Er II | 3 | ... | <1.19 | <-2.09 | <-3.01 | <1.37 | <-2.09 | Er II |
Tm II | 2 | ... | <1.48 | <-2.62 | <-2.74 | <1.64 | <-2.62 | Tm II |
Hf II | 2 | ... | <2.14 | <-1.21 | <-1.92 | <2.46 | <-1.21 | Hf II |
Ir I | 1 | ... | <2.33 | <-0.67 | <-2.05 | <2.33 | <-0.67 | Ir I |
Pb I | 1 | ... | <2.66 | <0.32 | <-1.72 | <2.66 | <0.32 | Pb I |
Th II | 2 | ... | <1.95 | <-2.19 | <-2.25 | <2.13 | <-2.19 | Th II |
Isotopic Ratio
Binary Parameters
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-8-06-8:32 | 2453953.86 | MIKELCO | 41000 | 65-135 | 5000 | -125.4 |
2009-7-25-8:04 | 2455037.84 | MIKELCO | 41000 | 65-135 | 1350 | -125.3 |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 4630+-34 | log g : 0.95+-0.13 | vturb : 1.7+-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 | ... | ... | <0.13 | <-3.13 | <1.25 | <0.13 | Li I |
CH | 1 | ... | 0.99+-0.25 | 5.21 | -3.22 | 1.16+-0.25 | 5.21 | CH |
NH | 1 | ... | 2.50+-0.36 | 6.12 | -1.71 | 2.67+-0.36 | 6.12 | NH |
O I | 2 | ... | <2.39 | <6.70 | <-1.99 | <2.39 | <6.70 | O I |
Mg I | 7 | ... | 1.56+-0.15 | 4.78 | -2.82 | 1.56+-0.15 | 4.78 | Mg I |
Al I | 1 | ... | 0.26+-0.29 | 2.33 | -4.12 | 0.26+-0.29 | 2.33 | Al I |
Si I | 1 | ... | 1.52+-0.28 | 4.65 | -2.86 | 1.52+-0.28 | 4.65 | Si I |
Ca I | 9 | ... | 0.67+-0.18 | 2.63 | -3.71 | 0.67+-0.18 | 2.63 | Ca I |
Sc II | 5 | ... | -0.14+-0.16 | -1.20 | -4.35 | 0.03+-0.16 | -1.20 | Sc II |
Ti I | 3 | ... | 0.28+-0.17 | 0.85 | -4.10 | 0.28+-0.17 | 0.85 | Ti I |
Ti II | 14 | ... | 0.19+-0.15 | 0.94 | -4.01 | 0.37+-0.15 | 0.94 | Ti II |
V II | 2 | ... | <0.46 | <0.19 | <-3.74 | <0.64 | <0.19 | V II |
Cr I | 4 | ... | -0.39+-0.15 | 0.87 | -4.77 | -0.39+-0.15 | 0.87 | Cr I |
Mn I | 3 | ... | -0.64+-0.14 | 0.41 | -5.02 | -0.64+-0.14 | 0.41 | Mn I |
Fe I | 58 | -4.38+-0.15 | ... | 3.12 | -4.38+-0.15 | ... | 3.12 | Fe I |
Fe II | 2 | -4.20+-0.16 | ... | 3.30 | -4.20+-0.16 | ... | 3.30 | Fe II |
Co I | 3 | ... | 0.19+-0.18 | 0.81 | -4.18 | 0.20+-0.18 | 0.81 | Co I |
Ni I | 6 | ... | 0.10+-0.23 | 1.94 | -4.28 | 0.10+-0.23 | 1.94 | Ni I |
Zn I | 2 | ... | <1.22 | <1.40 | <-3.16 | <1.22 | <1.40 | Zn I |
Rb I | 1 | ... | <3.51 | <1.65 | <-0.71 | <3.67 | <1.65 | Rb I |
Sr II | 2 | ... | 0.31+-0.25 | -1.02 | -3.89 | 0.49+-0.25 | -1.02 | Sr II |
Y II | 2 | ... | -0.25+-0.19 | -2.25 | -4.46 | -0.08+-0.19 | -2.25 | Y II |
Zr II | 2 | ... | 0.48+-0.19 | -1.15 | -3.73 | 0.65+-0.19 | -1.15 | Zr II |
Nb II | 1 | ... | <2.64 | <-0.10 | <-1.56 | <2.82 | <-0.10 | Nb II |
Mo I | 1 | ... | <1.98 | <-0.52 | <-2.40 | <1.98 | <-0.52 | Mo I |
Sn I | 1 | ... | <3.21 | <0.90 | <-1.17 | <3.21 | <0.90 | Sn I |
Ba II | 2 | ... | -0.78+-0.16 | -2.80 | -4.98 | -0.60+-0.16 | -2.80 | Ba II |
Ce II | 5 | ... | <0.74 | <-1.88 | <-3.46 | <0.92 | <-1.88 | Ce II |
Pr II | 4 | ... | <1.24 | <-2.24 | <-2.96 | <1.42 | <-2.24 | Pr II |
Nd II | 5 | ... | <0.65 | <-2.13 | <-3.55 | <0.83 | <-2.13 | Nd II |
Sm II | 2 | ... | <1.26 | <-1.98 | <-2.94 | <1.44 | <-1.98 | Sm II |
Eu II | 4 | ... | <0.51 | <-3.17 | <-3.69 | <0.69 | <-3.17 | Eu II |
Gd II | 1 | ... | <1.79 | <-1.34 | <-2.41 | <1.97 | <-1.34 | Gd II |
Tb II | 3 | ... | <1.48 | <-2.42 | <-2.74 | <1.64 | <-2.42 | Tb II |
Dy II | 3 | ... | <0.85 | <-2.25 | <-3.35 | <1.03 | <-2.25 | Dy II |
Ho II | 2 | ... | <1.36 | <-2.36 | <-2.83 | <1.55 | <-2.36 | Ho II |
Er II | 3 | ... | <1.19 | <-2.09 | <-3.01 | <1.37 | <-2.09 | Er II |
Tm II | 2 | ... | <1.48 | <-2.62 | <-2.74 | <1.64 | <-2.62 | Tm II |
Hf II | 2 | ... | <2.14 | <-1.21 | <-1.92 | <2.46 | <-1.21 | Hf II |
Ir I | 1 | ... | <2.33 | <-0.67 | <-2.05 | <2.33 | <-0.67 | Ir I |
Pb I | 1 | ... | <2.66 | <0.32 | <-1.72 | <2.66 | <0.32 | Pb I |
Th II | 2 | ... | <1.95 | <-2.19 | <-2.25 | <2.13 | <-2.19 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | -125.4 |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-08-06-08:32 | 2453953.86 | MIKELCO | 41000 | 65-135 | 5000 | -125.4 |
2009-07-25-08:04 | 2455037.84 | MIKELCO | 41000 | 65-135 | 1350 | -125.3 |
Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars
Stellar Parameters
Teff : 4900+-100 | log g : 1.5+-0.2 | vturb : 1.8+-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 | -3.97 | ... | ... | -3.97 | ... | 3.53 | Fe |
Sr | N/A | ... | 0.12+-0.2 | -0.95+-0.2 | -3.82+-0.2 | 0.15+-0.2 | -0.95+-0.2 | Sr |
Y | N/A | ... | -0.03+-0.2 | -1.80+-0.2 | -4.01+-0.2 | -0.04+-0.2 | -1.80+-0.2 | Y |
Zr | N/A | ... | 0.53+-0.2 | -0.87+-0.2 | -3.45+-0.2 | 0.52+-0.2 | -0.87+-0.2 | Zr |
Mo | N/A | ... | 1.33+-0.25 | -0.70+-0.25 | -2.58+-0.25 | 1.39+-0.25 | -0.70+-0.25 | Mo |
Pd | N/A | ... | 1.10+-0.25 | -1.20+-0.25 | -2.77+-0.25 | 1.20+-0.25 | -1.20+-0.25 | Pd |
Ba | N/A | ... | -0.73 | -2.52 | -4.70 | -0.73 | -2.52 | Ba |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.03 | 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 | 135 | N/A | N/A |
Binarity among CEMP-no stars: an indication of multiple formation pathways?
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 | ... | 1.16 | 5.97 | -2.46 | 1.92 | 5.97 | C |
Fe | N/A | -4.38 | ... | ... | -4.38 | ... | 3.12 | Fe |
Ba | N/A | ... | -0.6 | ... | -4.98 | -0.60 | -2.80 | Ba |
Binary Parameters
Binarity | Negative |
Vrad | -125.74+-0.29 |
Position
Right Ascension : 23 26 29.8 | Declination : -02 39 58 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2013-08-17-004311 | 2456521.53 | GECKOCFHT | 68000 | N/A | N/A | -126.1+-0.44 |
2013-08-28-005736 | 2456532.54 | GECKOCFHT | 68000 | N/A | N/A | -126.12+-0.41 |
2013-09-14-000000 | 2456549.5 | GECKOCFHT | 68000 | N/A | N/A | -126.05+-0.56 |
2014-06-08-020935 | 2456816.59 | GECKOCFHT | 68000 | N/A | N/A | -125.67+-0.32 |
2014-06-16-005736 | 2456824.54 | GECKOCFHT | 68000 | N/A | N/A | -126.1+-0.36 |
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 | ... | 2.16 | ... | -1.74 | 2.25 | 4.50 | Na |
Mg | N/A | ... | 1.2 | ... | -2.81 | 1.18 | 4.79 | Mg |
Ca | N/A | ... | 0.9 | ... | -3.07 | 0.92 | 3.27 | Ca |
Ti | N/A | ... | 0.53 | ... | -3.39 | 0.60 | 1.56 | Ti |
Fe | N/A | -3.99 | ... | ... | -3.99 | ... | 3.51 | Fe |
Ba | N/A | ... | -0.28 | ... | -4.32 | -0.33 | -2.14 | Ba |
Position
Right Ascension : 23 26 29.80 | Declination : -02 39 58.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log