CS22878-101
taken from 20 paper(s):
/R.Cayrel et al.(2004)/
/M.Spite et al.(2005)/
/E.Carretta et al.(2002)/
/J.G.Cohen et al.(2002)/
/A.McWilliam et al.(1995)/
/A.McWilliam et al.(1995)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/D.K.Lai et al.(2007)/
/S.M.Andrievsky et al.(2008)/
/Y.Ishimaru et al.(2004)/
/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)/
/J.G.Cohen et al.(2013)/
/I.U.Roederer et al.(2014)/
/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 : 4800 | log g : 1.3 | 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 | ... | ... | 5.00 | -3.43 | -0.14 | 5.00 | CH |
Na I | 2 | -3.11 | 0.14 | 3.22 | -3.02 | 0.27 | 3.22 | Na I |
Mg I | 7 | -2.81+-0.11 | 0.44+-0.11 | 4.77+-0.11 | -2.83+-0.11 | 0.46+-0.11 | 4.77+-0.11 | Mg I |
Al I | 2 | -4.01 | -0.76 | 2.46 | -3.99 | -0.70 | 2.46 | Al I |
Si I | 1 | -2.90 | 0.35 | 4.65 | -2.86 | 0.43 | 4.65 | Si I |
Ca I | 17 | -2.89+-0.16 | 0.36+-0.16 | 3.47+-0.16 | -2.87+-0.16 | 0.42+-0.16 | 3.47+-0.16 | Ca I |
Sc II | 7 | -3.13+-0.03 | 0.12+-0.03 | 0.04+-0.03 | -3.11+-0.03 | 0.18+-0.03 | 0.04+-0.03 | Sc II |
Ti I | 14 | -2.96+-0.14 | 0.29+-0.14 | 2.06+-0.14 | -2.89+-0.14 | 0.40+-0.14 | 2.06+-0.14 | Ti I |
Ti II | 28 | -3.00+-0.09 | 0.25+-0.09 | 2.02+-0.09 | -2.93+-0.09 | 0.36+-0.09 | 2.02+-0.09 | Ti II |
Cr I | 7 | -3.66+-0.13 | -0.41+-0.13 | 2.01+-0.13 | -3.63+-0.13 | -0.34+-0.13 | 2.01+-0.13 | Cr I |
Mn I | 3 | -3.79+-0.12 | -0.54+-0.12 | 1.60+-0.12 | -3.83+-0.12 | -0.54+-0.12 | 1.60+-0.12 | Mn I |
Fe I | 144 | -3.29+-0.12 | -0.04+-0.12 | 4.21+-0.12 | -3.29+-0.12 | -0.04+-0.12 | 4.21+-0.12 | Fe I |
Fe II | 17 | -3.21+-0.14 | 0.04+-0.14 | 4.29+-0.14 | -3.21+-0.14 | 0.04+-0.14 | 4.29+-0.14 | Fe II |
Co I | 4 | -3.03+-0.07 | 0.22+-0.07 | 1.89+-0.07 | -3.10+-0.07 | 0.19+-0.07 | 1.89+-0.07 | Co I |
Ni I | 3 | -3.48+-0.10 | -0.23+-0.10 | 2.77+-0.10 | -3.45+-0.10 | -0.16+-0.10 | 2.77+-0.10 | Ni I |
Zn I | 1 | -2.85 | 0.40 | 1.75 | -2.81 | 0.48 | 1.75 | Zn I |
Binary Parameters
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07 | N/A | VLT | 47000 | 85 | 14400 | 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 : 4800 | log g : 1.3 | 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 |
Li I | N/A | ... | ... | <-0.30 | <-3.56 | <-0.31 | <-0.30 | Li I |
C | N/A | -3.54+-0.10 | ... | ... | -3.45+-0.10 | -0.20+-0.10 | 4.98+-0.10 | C |
N | N/A | -1.92 | ... | ... | -1.83 | 1.42 | 6.00 | N |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 |
STELLAR ARCHAEOLOGY: A KECK PILOT PROGRAM ON EXTREMELY METAL-POOR STARS FROM THE HAMBURG/ESO SURVEY. II. ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 4775 | log g : 1.30 | vturb : 2.01 |
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 | 5 | ... | 0.68+-0.20 | ... | -2.41+-0.20 | 0.65+-0.20 | 5.19+-0.20 | Mg I |
Al I | 2 | ... | -0.59+-0.06 | ... | -3.64+-0.06 | -0.58+-0.06 | 2.81+-0.06 | Al I |
Si I | 1 | ... | 0.39 | ... | -2.64 | 0.42 | 4.87 | Si I |
Ca I | 7 | ... | 0.32+-0.08 | ... | -2.73+-0.08 | 0.33+-0.08 | 3.61+-0.08 | Ca I |
Sc II | 3 | ... | 0.22+-0.11 | ... | -2.91+-0.11 | 0.15+-0.11 | 0.24+-0.11 | Sc II |
Ti I | 13 | ... | 0.23+-0.10 | ... | -2.80+-0.10 | 0.26+-0.10 | 2.15+-0.10 | Ti I |
Ti II | 20 | ... | 0.24+-0.17 | ... | -2.79+-0.17 | 0.27+-0.17 | 2.16+-0.17 | Ti II |
Cr I | 9 | ... | -0.32+-0.24 | ... | -3.36+-0.24 | -0.30+-0.24 | 2.28+-0.24 | Cr I |
Mn I | 3 | ... | -1.05+-0.16 | ... | -4.16+-0.16 | -1.10+-0.16 | 1.27+-0.16 | Mn I |
Fe I | 44 | -3.07+-0.11 | ... | ... | -3.06+-0.11 | ... | 4.44+-0.11 | Fe I |
Fe II | 6 | -3.13+-0.09 | ... | ... | -3.12+-0.09 | ... | 4.38+-0.09 | Fe II |
Sr II | 2 | ... | -0.39+-0.13 | ... | -3.43+-0.13 | -0.37+-0.13 | -0.56+-0.13 | Sr II |
Ba II | 1 | ... | -1.08 | ... | -4.20 | -1.14 | -2.02 | Ba II |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 | N/A | KECKHIRES | 45000 | N/A | N/A | N/A |
STELLAR ARCHAEOLOGY: A KECK PILOT PROGRAM ON EXTREMELY METAL-POOR STARS FROM THE HAMBURG/ESO SURVEY. I. STELLAR PARAMETERS
Stellar Parameters
Binary Parameters
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 | N/A | KECKHIRES | 45000 | 96 | 3600 | |
A Spectroscopic Analysis of 33 of the Most Metal-Poor Stars.I.
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 : 4790 | log g : 1.15+-0.26 | vturb : 2.39+-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 |
C | N/A | ... | -0.30 | ... | -3.30 | -0.34 | 5.13 | C |
Na | N/A | ... | -0.09 | ... | -3.13 | -0.17 | 3.11 | Na |
Mg | N/A | ... | 0.43 | ... | -2.72 | 0.24 | 4.88 | Mg |
Ca | N/A | ... | 0.42 | ... | -2.69 | 0.27 | 3.65 | Ca |
Fe I | N/A | -3.13 | ... | ... | -2.96 | ... | 4.54 | Fe I |
Fe II | N/A | -3.13 | ... | ... | -2.96 | ... | 4.54 | Fe II |
Ni | N/A | ... | 0.23 | ... | -2.87 | 0.09 | 3.35 | Ni |
Sr | N/A | ... | -0.50 | ... | -3.60 | -0.64 | -0.73 | Sr |
Ba | N/A | ... | -0.65 | ... | -3.83 | -0.87 | -1.65 | Ba |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 : 4800 | log g : 1.3 | 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 |
C | N/A | -3.46+-0.10 | ... | ... | -3.37+-0.10 | -0.12+-0.10 | 5.06+-0.10 | C |
N | N/A | -1.92+-0.10 | ... | ... | -1.83+-0.10 | 1.42+-0.10 | 6.00+-0.10 | N |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Isotopic Ratio
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 : 4800 | log g : 1.3 | 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 |
Na | N/A | -3.30 | -0.05 | 2.95 | -3.29 | -0.04 | 2.95 | Na |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 |
Carbon and Strontium Abundances of 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 | ... | -0.45+-0.19 | ... | -3.25+-0.19 | -0.49+-0.19 | 5.18+-0.19 | C |
Fe | N/A | -2.93 | ... | ... | -2.76 | ... | 4.74 | Fe |
Sr | N/A | ... | -0.07 | ... | -2.97 | -0.21 | -0.10 | Sr |
Ba | N/A | ... | -0.53 | ... | -3.51 | -0.75 | -1.33 | Ba |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 | KECKII | 7000 | N/A | N/A | N/A |
NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4800 | log g : 1.3 | 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 |
Al | N/A | -3.37 | -0.12 | 3.10 | -3.35 | -0.10 | 3.10 | Al |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 | 120 | N/A | N/A |
The Detection of Low Eu Abundances in Extremely Metal-poor Stars and the Origin of r-Process Elements
Stellar Parameters
Teff : 4775 | log g : 1.3 | 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 |
Fe I | 161 | -3.14+-0.14 | ... | +4.36+-0.14 | -3.14+-0.14 | ... | +4.36+-0.14 | Fe I |
Fe II | 20 | -3.07+-0.14 | ... | +4.43+-0.14 | -3.07+-0.14 | ... | +4.43+-0.14 | Fe II |
Sr II | 2 | ... | -0.15+-0.28 | -0.33+-0.28 | -3.20+-0.28 | -0.06+-0.28 | -0.33+-0.28 | Sr II |
Ba II | 2 | ... | -0.73+-0.16 | -1.61+-0.16 | -3.79+-0.16 | -0.65+-0.16 | -1.61+-0.16 | Ba II |
Eu II | 2 | ... | -0.30+-0.24 | -2.85+-0.24 | -3.37+-0.24 | -0.23+-0.24 | -2.85+-0.24 | Eu II |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-07 | N/A | SUBARUHDS | 50000 | N/A | 14400 | 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 : 4800 | log g : 1.3 | 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 |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Ba | 2 | ... | ... | -1.70 | -3.88 | -0.63 | -1.70 | Ba |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 : 4800 | log g : 1.3 | 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 |
Mg | N/A | ... | ... | 4.85 | -2.75 | 0.50 | 4.85 | Mg |
K | N/A | ... | ... | 2.35 | -2.68 | 0.57 | 2.35 | K |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 : 4800 | log g : 1.3 | 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 |
S I | 1 | ... | ... | 4.55+-0.16 | -2.57+-0.16 | 0.68+-0.16 | 4.55+-0.16 | S I |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 | 180 | N/A | N/A |
First stars. VIII. Enrichment of the neutron-capture elements in the early Galaxy
Stellar Parameters
Teff : 4800 | log g : 1.3 | 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 |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Sr | 2 | ... | -0.27 | ... | -3.47 | -0.22 | -0.60 | Sr |
Y | 9 | ... | -0.28 | ... | -3.50 | -0.25 | -1.29 | Y |
Zr | 6 | ... | +0.05 | ... | -3.18 | 0.07 | -0.60 | Zr |
Ba | 2 | ... | -0.58 | ... | -3.88 | -0.63 | -1.70 | Ba |
La | 1 | ... | -0.42 | ... | -3.60 | -0.35 | -2.50 | La |
Ce | N/A | ... | <+0.17 | ... | <-3.08 | <0.17 | <-1.50 | Ce |
Pr | N/A | ... | <+0.09 | ... | <-3.17 | <0.08 | <-2.45 | Pr |
Nd | N/A | ... | <-0.45 | ... | <-3.62 | <-0.37 | <-2.20 | Nd |
Sm | N/A | ... | <+0.34 | ... | <-2.86 | <0.39 | <-1.90 | Sm |
Eu | 1 | ... | -0.06 | ... | -3.32 | -0.07 | -2.80 | Eu |
Gd | N/A | ... | <-0.07 | ... | <-3.27 | <-0.02 | <-2.20 | Gd |
Dy | 1 | ... | -0.29 | ... | -3.50 | -0.25 | -2.40 | Dy |
Ho | N/A | ... | <+0.19 | ... | <-3.27 | <-0.02 | <-2.80 | Ho |
Er | N/A | ... | <+0.02 | ... | <-3.22 | <0.03 | <-2.30 | Er |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 | >50 | N/A | N/A |
NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
Stellar Parameters
Teff : 4800 | log g : 1.3 | 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 |
Ca | N/A | -2.68 | 0.57 | ... | -2.66 | 0.59 | 3.68 | Ca |
Fe | N/A | -3.25 | ... | ... | -3.25 | ... | 4.25 | Fe |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Stellar Parameters
Teff : 4775 | log g : 1.3 | vturb : 2 |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | 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 | N/A | KECKHIRES | 36000 | 125 | 2400 | -131.7 |
Neutron-capture Nucleosynthesis in the First Stars
Stellar Parameters
Teff : 4650+-35 | log g : 1.05+-0.14 | vturb : 1.90+-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 | ... | ... | <0.43 | <-2.83 | <0.70 | <0.43 | Li I |
CH | 1 | ... | -0.60+-0.25 | 4.53+-0.25 | -3.90+-0.25 | -0.37+-0.25 | 4.53+-0.25 | CH |
NH | 1 | ... | 1.29+-0.36 | 5.48+-0.36 | -2.35+-0.36 | 1.18+-0.36 | 5.48+-0.36 | NH |
O I | 1 | ... | 1.23+-0.20 | 6.39+-0.20 | -2.30+-0.20 | 1.23+-0.20 | 6.39+-0.20 | O I |
Mg I | 8 | ... | 0.60+-0.16 | 4.67+-0.16 | -2.93+-0.16 | 0.60+-0.16 | 4.67+-0.16 | Mg I |
Al I | 1 | ... | -0.59+-0.30 | 2.33+-0.30 | -4.12+-0.30 | -0.59+-0.30 | 2.33+-0.30 | Al I |
Si I | 1 | ... | 0.82+-0.29 | 4.80+-0.29 | -2.71+-0.29 | 0.82+-0.29 | 4.80+-0.29 | Si I |
Ca I | 13 | ... | 0.49+-0.17 | 3.30+-0.17 | -3.04+-0.17 | 0.49+-0.17 | 3.30+-0.17 | Ca I |
Sc II | 6 | ... | -0.05+-0.15 | -0.19+-0.15 | -3.34+-0.15 | 0.19+-0.15 | -0.19+-0.15 | Sc II |
Ti I | 10 | ... | 0.33+-0.14 | 1.75+-0.14 | -3.20+-0.14 | 0.33+-0.14 | 1.75+-0.14 | Ti I |
Ti II | 24 | ... | 0.23+-0.14 | 1.89+-0.14 | -3.06+-0.14 | 0.47+-0.14 | 1.89+-0.14 | Ti II |
V I | 1 | ... | -0.02+-0.18 | 0.38+-0.18 | -3.55+-0.18 | -0.02+-0.18 | 0.38+-0.18 | V I |
V II | 2 | ... | 0.04+-0.24 | 0.67+-0.24 | -3.26+-0.24 | 0.27+-0.24 | 0.67+-0.24 | V II |
Cr I | 5 | ... | -0.24+-0.15 | 1.87+-0.15 | -3.77+-0.15 | -0.24+-0.15 | 1.87+-0.15 | Cr I |
Cr II | 1 | ... | 0.07+-0.17 | 2.41+-0.17 | -3.23+-0.17 | 0.30+-0.17 | 2.41+-0.17 | Cr II |
Mn I | 4 | ... | -0.50+-0.17 | 1.41+-0.17 | -4.02+-0.17 | -0.49+-0.17 | 1.41+-0.17 | Mn I |
Mn II | 2 | ... | -0.76+-0.21 | 1.37+-0.21 | -4.06+-0.21 | -0.53+-0.21 | 1.37+-0.21 | Mn II |
Fe I | 100 | -3.53+-0.15 | ... | 3.97+-0.15 | -3.53+-0.15 | ... | 3.97+-0.15 | Fe I |
Fe II | 11 | -3.30+-0.15 | ... | 4.20+-0.15 | -3.30+-0.15 | ... | 4.20+-0.15 | Fe II |
Co I | 3 | ... | -0.01+-0.19 | 1.45+-0.19 | -3.54+-0.19 | -0.01+-0.19 | 1.45+-0.19 | Co I |
Ni I | 3 | ... | -0.01+-0.19 | 2.69+-0.19 | -3.53+-0.19 | 0.00+-0.19 | 2.69+-0.19 | Ni I |
Zn I | 2 | ... | 0.62+-0.15 | 1.66+-0.15 | -2.90+-0.15 | 0.63+-0.15 | 1.66+-0.15 | Zn I |
Rb I | 1 | ... | <2.52 | <1.51 | <-0.85 | <2.68 | <1.51 | Rb I |
Sr II | 2 | ... | -0.35+-0.25 | -0.78+-0.25 | -3.65+-0.25 | -0.12+-0.25 | -0.78+-0.25 | Sr II |
Y II | 4 | ... | -0.67+-0.18 | -1.76+-0.18 | -3.97+-0.18 | -0.44+-0.18 | -1.76+-0.18 | Y II |
Zr II | 3 | ... | -0.07+-0.16 | -0.79+-0.16 | -3.37+-0.16 | 0.16+-0.16 | -0.79+-0.16 | Zr II |
Nb II | 1 | ... | <1.99 | <0.15 | <-1.31 | <2.22 | <0.15 | Nb II |
Mo I | 1 | ... | <1.36 | <-0.29 | <-2.17 | <1.36 | <-0.29 | Mo I |
Tc I | 1 | ... | ... | <-0.13 | <-0.13 | <3.40 | <-0.13 | Tc I |
Sn I | 1 | ... | <2.27 | <0.81 | <-1.26 | <2.27 | <0.81 | Sn I |
Ba II | 3 | ... | -0.60+-0.15 | -1.72+-0.15 | -3.90+-0.15 | -0.37+-0.15 | -1.72+-0.15 | Ba II |
La II | 1 | ... | -0.27+-0.22 | -2.47+-0.22 | -3.57+-0.22 | -0.04+-0.22 | -2.47+-0.22 | La II |
Ce II | 5 | ... | <-0.04 | <-1.76 | <-3.34 | <0.19 | <-1.76 | Ce II |
Pr II | 1 | ... | <0.23 | <-2.35 | <-3.07 | <0.46 | <-2.35 | Pr II |
Nd II | 1 | ... | -0.38+-0.25 | -2.26+-0.25 | -3.68+-0.25 | -0.15+-0.25 | -2.26+-0.25 | Nd II |
Sm II | 2 | ... | <0.56 | <-1.78 | <-2.74 | <0.79 | <-1.78 | Sm II |
Eu II | 4 | ... | <-0.27 | <-3.05 | <-3.57 | <-0.04 | <-3.05 | Eu II |
Gd II | 3 | ... | <0.83 | <-1.40 | <-2.47 | <1.06 | <-1.40 | Gd II |
Tb II | 3 | ... | <0.77 | <-2.23 | <-2.55 | <0.98 | <-2.23 | Tb II |
Dy II | 3 | ... | <-0.01 | <-2.21 | <-3.31 | <0.22 | <-2.21 | Dy II |
Ho II | 1 | ... | <0.60 | <-2.22 | <-2.69 | <0.84 | <-2.22 | Ho II |
Er II | 2 | ... | <0.33 | <-2.05 | <-2.97 | <0.56 | <-2.05 | Er II |
Tm II | 2 | ... | <0.82 | <-2.38 | <-2.50 | <1.03 | <-2.38 | Tm II |
Hf II | 2 | ... | <1.19 | <-1.26 | <-1.97 | <1.56 | <-1.26 | Hf II |
Ir I | 1 | ... | <1.51 | <-0.64 | <-2.02 | <1.51 | <-0.64 | Ir I |
Pb I | 1 | ... | <1.81 | <0.32 | <-1.72 | <1.81 | <0.32 | Pb I |
Th II | 2 | ... | <0.98 | <-2.26 | <-2.32 | <1.21 | <-2.26 | Th II |
Binary Parameters
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-8-05-23:59 | 2453953.501 | MIKELCO | 41000 | 60-115 | 2400 | -128.8 |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 4650+-35 | log g : 1.05+-0.14 | vturb : 1.9+-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 | ... | ... | <0.43 | <-2.83 | <0.70 | <0.43 | Li I |
CH | 1 | ... | -0.60+-0.25 | 4.53 | -3.90 | -0.37+-0.25 | 4.53 | CH |
NH | 1 | ... | 1.29+-0.36 | 5.48 | -2.35 | 1.18+-0.36 | 5.48 | NH |
O I | 1 | ... | 1.23+-0.20 | 6.39 | -2.30 | 1.23+-0.20 | 6.39 | O I |
Mg I | 8 | ... | 0.60+-0.16 | 4.67 | -2.93 | 0.60+-0.16 | 4.67 | Mg I |
Al I | 1 | ... | -0.59+-0.30 | 2.33 | -4.12 | -0.59+-0.30 | 2.33 | Al I |
Si I | 1 | ... | 0.82+-0.29 | 4.80 | -2.71 | 0.82+-0.29 | 4.80 | Si I |
Ca I | 13 | ... | 0.49+-0.17 | 3.30 | -3.04 | 0.49+-0.17 | 3.30 | Ca I |
Sc II | 6 | ... | -0.05+-0.15 | -0.19 | -3.34 | 0.19+-0.15 | -0.19 | Sc II |
Ti I | 10 | ... | 0.33+-0.14 | 1.75 | -3.20 | 0.33+-0.14 | 1.75 | Ti I |
Ti II | 24 | ... | 0.23+-0.14 | 1.89 | -3.06 | 0.47+-0.14 | 1.89 | Ti II |
V I | 1 | ... | -0.02+-0.18 | 0.38 | -3.55 | -0.02+-0.18 | 0.38 | V I |
V II | 2 | ... | 0.04+-0.24 | 0.67 | -3.26 | 0.27+-0.24 | 0.67 | V II |
Cr I | 5 | ... | -0.24+-0.15 | 1.87 | -3.77 | -0.24+-0.15 | 1.87 | Cr I |
Cr II | 1 | ... | 0.07+-0.17 | 2.41 | -3.23 | 0.30+-0.17 | 2.41 | Cr II |
Mn I | 4 | ... | -0.50+-0.17 | 1.41 | -4.02 | -0.49+-0.17 | 1.41 | Mn I |
Mn II | 2 | ... | -0.76+-0.21 | 1.37 | -4.06 | -0.53+-0.21 | 1.37 | Mn II |
Fe I | 100 | -3.53+-0.15 | ... | 3.97 | -3.53+-0.15 | ... | 3.97 | Fe I |
Fe II | 11 | -3.30+-0.15 | ... | 4.20 | -3.30+-0.15 | ... | 4.20 | Fe II |
Co I | 3 | ... | -0.01+-0.19 | 1.45 | -3.54 | -0.01+-0.19 | 1.45 | Co I |
Ni I | 3 | ... | -0.01+-0.19 | 2.69 | -3.53 | 0.00+-0.19 | 2.69 | Ni I |
Zn I | 2 | ... | 0.62+-0.15 | 1.66 | -2.90 | 0.63+-0.15 | 1.66 | Zn I |
Rb I | 1 | ... | <2.52 | <1.51 | <-0.85 | <2.68 | <1.51 | Rb I |
Sr II | 2 | ... | -0.35+-0.25 | -0.78 | -3.65 | -0.12+-0.25 | -0.78 | Sr II |
Y II | 4 | ... | -0.67+-0.18 | -1.76 | -3.97 | -0.44+-0.18 | -1.76 | Y II |
Zr II | 3 | ... | -0.07+-0.16 | -0.79 | -3.37 | 0.16+-0.16 | -0.79 | Zr II |
Nb II | 1 | ... | <1.99 | <0.15 | <-1.31 | <2.22 | <0.15 | Nb II |
Mo I | 1 | ... | <1.36 | <-0.29 | <-2.17 | <1.36 | <-0.29 | Mo I |
Tc I | 1 | ... | ... | <-0.13 | <-0.13 | <3.40 | <-0.13 | Tc I |
Sn I | 1 | ... | <2.27 | <0.81 | <-1.26 | <2.27 | <0.81 | Sn I |
Ba II | 3 | ... | -0.60+-0.15 | -1.72 | -3.90 | -0.37+-0.15 | -1.72 | Ba II |
La II | 1 | ... | -0.27+-0.22 | -2.47 | -3.57 | -0.04+-0.22 | -2.47 | La II |
Ce II | 5 | ... | <-0.04 | <-1.76 | <-3.34 | <0.19 | <-1.76 | Ce II |
Pr II | 1 | ... | <0.23 | <-2.35 | <-3.07 | <0.46 | <-2.35 | Pr II |
Nd II | 1 | ... | -0.38+-0.25 | -2.26 | -3.68 | -0.15+-0.25 | -2.26 | Nd II |
Sm II | 2 | ... | <0.56 | <-1.78 | <-2.74 | <0.79 | <-1.78 | Sm II |
Eu II | 4 | ... | <-0.27 | <-3.05 | <-3.57 | <-0.04 | <-3.05 | Eu II |
Gd II | 3 | ... | <0.83 | <-1.40 | <-2.47 | <1.06 | <-1.40 | Gd II |
Tb II | 3 | ... | <0.77 | <-2.23 | <-2.55 | <0.98 | <-2.23 | Tb II |
Dy II | 3 | ... | <-0.01 | <-2.21 | <-3.31 | <0.22 | <-2.21 | Dy II |
Ho II | 1 | ... | <0.60 | <-2.22 | <-2.69 | <0.84 | <-2.22 | Ho II |
Er II | 2 | ... | <0.33 | <-2.05 | <-2.97 | <0.56 | <-2.05 | Er II |
Tm II | 2 | ... | <0.82 | <-2.38 | <-2.50 | <1.03 | <-2.38 | Tm II |
Hf II | 2 | ... | <1.19 | <-1.26 | <-1.97 | <1.56 | <-1.26 | Hf II |
Ir I | 1 | ... | <1.51 | <-0.64 | <-2.02 | <1.51 | <-0.64 | Ir I |
Pb I | 1 | ... | <1.81 | <0.32 | <-1.72 | <1.81 | <0.32 | Pb I |
Th II | 2 | ... | <0.98 | <-2.26 | <-2.32 | <1.21 | <-2.26 | Th II |
Binary Parameters
Binarity | Positive |
Vrad | -128.8 |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-08-05-23:59 | 2453953.501 | MIKELCO | 41000 | 60-115 | 2400 | -128.8 |
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 | ... | -0.09 | ... | -3.13 | 0.00 | 3.11 | Na |
Mg | N/A | ... | 0.43 | ... | -2.72 | 0.41 | 4.88 | Mg |
Ca | N/A | ... | 0.42 | ... | -2.69 | 0.44 | 3.65 | Ca |
Ti | N/A | ... | 0.41 | ... | -2.65 | 0.48 | 2.30 | Ti |
Fe | N/A | -3.13 | ... | ... | -3.13 | ... | 4.37 | Fe |
Ni | N/A | ... | 0.23 | ... | -2.87 | 0.26 | 3.35 | Ni |
Y | N/A | ... | -0.55 | ... | -3.65 | -0.52 | -1.44 | Y |
Ba | N/A | ... | -0.87 | ... | -4.05 | -0.92 | -1.87 | Ba |
Position
Right Ascension : 16 45 31.40 | Declination : +08 14 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log