CS22885-096
taken from 15 paper(s):
/J.E.Norris et al.(2001)/
/R.Cayrel et al.(2004)/
/P.Francois et al.(2003)/
/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)/
/P.Francois et al.(2007)/
/M.Spite et al.(2012)/
/I.U.Roederer et al.(2014)/
/K.A.Venn et al.(2004)/
EXTREMELY METAL-POOR STARS. VIII. HIGH-RESOLUTION, HIGH SIGNAL-TO-NOISE RATIO ANALYSIS OF FIVE STARS WITH [Fe/H]<=-3.5
Stellar Parameters
Teff : 5050 | log g : 1.9 | 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 | ... | 0.60+-0.20 | ... | -2.82+-0.20 | 0.67+-0.20 | 5.61+-0.20 | CH |
Mg I | 5 | ... | 0.52+-0.08 | ... | -3.16+-0.08 | 0.33+-0.08 | 4.44+-0.08 | Mg I |
Al I | 1 | ... | -0.78+-0.21 | ... | -4.42+-0.21 | -0.93+-0.21 | 2.03+-0.21 | Al I |
Si I | 2 | ... | 0.44+-0.19 | ... | -3.18+-0.19 | 0.31+-0.19 | 4.33+-0.19 | Si I |
Ca I | 6 | ... | 0.28+-0.09 | ... | -3.36+-0.09 | 0.13+-0.09 | 2.98+-0.09 | Ca I |
Sc II | 6 | ... | 0.15+-0.16 | ... | -3.57+-0.16 | -0.08+-0.16 | -0.42+-0.16 | Sc II |
Ti I | 4 | ... | 0.21+-0.09 | ... | -3.41+-0.09 | 0.08+-0.09 | 1.54+-0.09 | Ti I |
Ti II | 25 | ... | 0.12+-0.15 | ... | -3.50+-0.15 | -0.01+-0.15 | 1.45+-0.15 | Ti II |
V II | 1 | ... | <0.31+-0.19 | ... | <-3.28+-0.19 | <0.21+-0.19 | <0.65+-0.19 | V II |
Cr I | 3 | ... | -0.59+-0.10 | ... | -4.22+-0.10 | -0.73+-0.10 | 1.42+-0.10 | Cr I |
Mn I | 3 | ... | -0.79+-0.10 | ... | -4.49+-0.10 | -1.00+-0.10 | 0.94+-0.10 | Mn I |
Fe I | 97 | -3.66+-0.15 | ... | ... | -3.49+-0.15 | ... | 4.01+-0.15 | Fe I |
Fe II | 3 | -3.67+-0.23 | ... | ... | -3.50+-0.23 | ... | 4.00+-0.23 | Fe II |
Co I | 5 | ... | 0.59+-0.11 | ... | -3.14+-0.11 | 0.35+-0.11 | 1.85+-0.11 | Co I |
Ni I | 5 | ... | 0.18+-0.08 | ... | -3.45+-0.08 | 0.04+-0.08 | 2.77+-0.08 | Ni I |
Sr II | 2 | ... | -1.59+-0.15 | ... | -5.22+-0.15 | -1.73+-0.15 | -2.35+-0.15 | Sr II |
Y II | 1 | ... | <-0.54+-0.15 | ... | <-4.17+-0.15 | <-0.68+-0.15 | <-1.96+-0.15 | Y II |
Ba II | 1 | ... | -1.44+-0.21 | ... | -5.15+-0.21 | -1.66+-0.21 | -2.97+-0.21 | Ba II |
Eu II | 1 | ... | <0.68+-0.18 | ... | <-2.99+-0.18 | <0.50+-0.18 | <-2.47+-0.18 | Eu II |
Binary Parameters
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-08-21 | N/A | ANGLO | 42000 | N/A | N/A | -251.0+-1.08 |
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Stellar Parameters
Teff : 5050 | log g : 2.6 | 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 | -3.57 | 0.24 | 4.95 | -3.48 | 0.33 | 4.95 | CH |
Na I | 2 | -3.84 | -0.06 | 2.49 | -3.75 | 0.06 | 2.49 | Na I |
Mg I | 7 | -3.59+-0.12 | 0.19+-0.12 | 3.99+-0.12 | -3.61+-0.12 | 0.20+-0.12 | 3.99+-0.12 | Mg I |
Al I | 2 | -4.57 | -0.79 | 1.90 | -4.55 | -0.74 | 1.90 | Al I |
Si I | 1 | -3.26 | 0.52 | 4.29 | -3.22 | 0.59 | 4.29 | Si I |
K I | 2 | -3.44 | 0.34 | 1.68 | -3.35 | 0.46 | 1.68 | K I |
Ca I | 12 | -3.43+-0.15 | 0.35+-0.15 | 2.93+-0.15 | -3.41+-0.15 | 0.40+-0.15 | 2.93+-0.15 | Ca I |
Sc II | 5 | -3.41+-0.08 | 0.37+-0.08 | -0.24+-0.08 | -3.39+-0.08 | 0.42+-0.08 | -0.24+-0.08 | Sc II |
Ti I | 9 | -3.44+-0.07 | 0.34+-0.07 | 1.58+-0.07 | -3.37+-0.07 | 0.44+-0.07 | 1.58+-0.07 | Ti I |
Ti II | 24 | -3.46+-0.11 | 0.32+-0.11 | 1.56+-0.11 | -3.39+-0.11 | 0.42+-0.11 | 1.56+-0.11 | Ti II |
Cr I | 7 | -4.26+-0.13 | -0.48+-0.13 | 1.41+-0.13 | -4.23+-0.13 | -0.42+-0.13 | 1.41+-0.13 | Cr I |
Mn I | 3 | -4.32+-0.02 | -0.54+-0.02 | 1.07+-0.02 | -4.36+-0.02 | -0.55+-0.02 | 1.07+-0.02 | Mn I |
Fe I | 120 | -3.81+-0.17 | -0.03+-0.17 | 3.69+-0.17 | -3.81+-0.17 | -0.03+-0.17 | 3.69+-0.17 | Fe I |
Fe II | 5 | -3.75+-0.14 | 0.03+-0.14 | 3.75+-0.14 | -3.75+-0.14 | 0.03+-0.14 | 3.75+-0.14 | Fe II |
Co I | 4 | -3.30+-0.05 | 0.48+-0.05 | 1.62+-0.05 | -3.37+-0.05 | 0.44+-0.05 | 1.62+-0.05 | Co I |
Ni I | 3 | -3.78+-0.06 | 0.00+-0.06 | 2.47+-0.06 | -3.75+-0.06 | 0.06+-0.06 | 2.47+-0.06 | Ni I |
Zn I | 1 | -3.34 | 0.44 | 1.26 | -3.30 | 0.51 | 1.26 | Zn I |
Binary Parameters
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 | 160 | 15835 | N/A |
2000-08 | N/A | VLT | N/A | N/A | N/A | N/A |
First Stars. III. A detailed elemental abundance study of four extremely metal-poor giant stars
Stellar Parameters
Teff : 4900 | log g : 2.0 | 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 I | 2 | -3.98+-0.04 | ... | ... | -3.89+-0.04 | 0.07+-0.04 | 2.35+-0.04 | Na I |
Mg I | 4 | -3.50+-0.36 | ... | ... | -3.52+-0.36 | 0.44+-0.36 | 4.08+-0.36 | Mg I |
Al I | 2 | -4.70+-0.03 | ... | ... | -4.68+-0.03 | -0.72+-0.03 | 1.77+-0.03 | Al I |
Si I | 1 | -3.55 | ... | ... | -3.51 | 0.45 | 4.00 | Si I |
Ca I | 12 | -3.48+-0.12 | ... | ... | -3.46+-0.12 | 0.50+-0.12 | 2.88+-0.12 | Ca I |
Sc II | 6 | -3.76+-0.19 | ... | ... | -3.74+-0.19 | 0.22+-0.19 | -0.59+-0.19 | Sc II |
Ti I | 9 | -3.61+-0.08 | ... | ... | -3.54+-0.08 | 0.42+-0.08 | 1.41+-0.08 | Ti I |
Cr I | 7 | -4.38+-0.16 | ... | ... | -4.35+-0.16 | -0.39+-0.16 | 1.29+-0.16 | Cr I |
Mn I | 5 | -4.56+-0.25 | ... | ... | -4.60+-0.25 | -0.64+-0.25 | 0.83+-0.25 | Mn I |
Fe I | 91 | -3.96+-0.11 | ... | ... | -3.96+-0.11 | ... | 3.54+-0.11 | Fe I |
Fe II | 5 | -3.95+-0.12 | ... | ... | -3.95+-0.12 | ... | 3.55+-0.12 | Fe II |
Co I | 4 | -3.48+-0.06 | ... | ... | -3.55+-0.06 | 0.41+-0.06 | 1.44+-0.06 | Co I |
Ni I | 3 | -3.98+-0.05 | ... | ... | -3.95+-0.05 | 0.01+-0.05 | 2.27+-0.05 | Ni I |
Sr II | 2 | -5.50+-0.00 | ... | ... | -5.45+-0.00 | -1.49+-0.00 | -2.58+-0.00 | Sr II |
Y II | 1 | -5.48 | ... | ... | -5.45 | -1.49 | -3.24 | Y II |
Ba II | 2 | -4.99 | ... | ... | -5.04 | -1.08 | -2.86 | Ba II |
Eu II | 1 | <-3.51 | ... | ... | <-3.52 | <0.44 | <-3.00 | Eu II |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 | 45000 | 160 | 15835 | N/A |
2000-08 | N/A | VLT | 45000 | 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 : 5050 | log g : 2.6 | 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 | ... | ... | 0.83+-0.05 | -2.43+-0.05 | 1.35+-0.05 | 0.83+-0.05 | Li I |
C | N/A | -3.52+-0.06 | ... | ... | -3.43+-0.06 | 0.35+-0.06 | 5.00+-0.06 | C |
N | N/A | -3.52 | ... | ... | -3.43 | 0.35 | 4.40 | N |
Fe | N/A | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 4920 | log g : 2.10+-0.34 | vturb : 2.15+-0.14 |
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 | ... | -3.36 | 0.26 | 5.07 | C |
Na | N/A | ... | -0.11 | ... | -3.81 | -0.19 | 2.43 | Na |
Mg | N/A | ... | 0.46 | ... | -3.35 | 0.27 | 4.25 | Mg |
Ca | N/A | ... | 0.58 | ... | -3.19 | 0.43 | 3.15 | Ca |
Fe I | N/A | -3.79 | ... | ... | -3.62 | ... | 3.88 | Fe I |
Fe II | N/A | -3.79 | ... | ... | -3.62 | ... | 3.88 | Fe II |
Ni | N/A | ... | 0.83 | ... | -2.93 | 0.69 | 3.29 | Ni |
Sr | N/A | ... | -1.35 | ... | -5.11 | -1.49 | -2.24 | Sr |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 5050 | log g : 2.6 | 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 | -3.52+-0.06 | ... | ... | -3.43+-0.06 | 0.35+-0.06 | 5.00+-0.06 | C |
N | N/A | -3.52+-0.13 | ... | ... | -3.43+-0.13 | 0.35+-0.13 | 4.40+-0.13 | N |
Fe | N/A | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 5050 | log g : 2.6 | 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 | -3.75 | +0.03 | 2.50 | -3.74 | 0.04 | 2.50 | Na |
Fe | N/A | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 5050 | log g : 2.6 | 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 |
Al | N/A | -3.67 | 0.11 | 2.80 | -3.65 | 0.13 | 2.80 | Al |
Fe | N/A | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 5050 | log g : 2.6 | 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 | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Ba | 1 | ... | ... | -2.75 | -4.93 | -1.15 | -2.75 | Ba |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 5050 | log g : 2.6 | 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 | ... | ... | 4.13 | -3.47 | 0.31 | 4.13 | Mg |
K | N/A | ... | ... | 1.80 | -3.23 | 0.55 | 1.80 | K |
Fe | N/A | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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. VIII. Enrichment of the neutron-capture elements in the early Galaxy
Stellar Parameters
Teff : 5050 | log g : 2.6 | 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 | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Sr | 2 | ... | -1.39 | ... | -5.12 | -1.34 | -2.25 | Sr |
Y | N/A | ... | <-0.86 | ... | <-4.61 | <-0.83 | <-2.40 | Y |
Zr | 1 | ... | -0.42 | ... | -4.18 | -0.40 | -1.60 | Zr |
Ba | 1 | ... | -1.10 | ... | -4.93 | -1.15 | -2.75 | Ba |
La | N/A | ... | <-0.09 | ... | <-3.80 | <-0.02 | <-2.70 | La |
Ce | N/A | ... | <+0.90 | ... | <-2.88 | <0.90 | <-1.30 | Ce |
Pr | N/A | ... | <+0.62 | ... | <-3.17 | <0.61 | <-2.45 | Pr |
Nd | N/A | ... | <+0.58 | ... | <-3.12 | <0.66 | <-1.70 | Nd |
Sm | N/A | ... | <+1.27 | ... | <-2.46 | <1.32 | <-1.50 | Sm |
Eu | N/A | ... | <+0.47 | ... | <-3.32 | <0.46 | <-2.80 | Eu |
Gd | N/A | ... | <+0.86 | ... | <-2.87 | <0.91 | <-1.80 | Gd |
Dy | N/A | ... | <+0.24 | ... | <-3.50 | <0.28 | <-2.40 | Dy |
Ho | N/A | ... | <+0.82 | ... | <-3.17 | <0.61 | <-2.70 | Ho |
Er | N/A | ... | <+0.55 | ... | <-3.22 | <0.56 | <-2.30 | Er |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 5050 | log g : 2.6 | 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 | -3.26 | 0.52 | ... | -3.24 | 0.54 | 3.10 | Ca |
Fe | N/A | -3.78 | ... | ... | -3.78 | ... | 3.72 | Fe |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | 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 : 4580+-34 | log g : 0.75+-0.15 | vturb : 1.75+-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 | 1.67 | 0.52 | Li I |
CH | 1 | ... | 0.40+-0.25 | 4.62 | -3.81 | 0.60+-0.25 | 4.62 | CH |
NH | 1 | ... | <1.38 | <5.00 | <-2.83 | <1.58 | <5.00 | NH |
O I | 3 | ... | <2.45 | <6.73 | <-1.96 | <2.45 | <6.73 | O I |
Na I | 1 | ... | 0.22+-0.18 | 2.05 | -4.19 | 0.22+-0.18 | 2.05 | Na I |
Mg I | 7 | ... | 0.83+-0.18 | 4.03 | -3.57 | 0.84+-0.18 | 4.03 | Mg I |
Al I | 1 | ... | -0.67+-0.18 | 1.37 | -5.08 | -0.67+-0.18 | 1.37 | Al I |
Si I | 1 | ... | 0.88+-0.33 | 3.98 | -3.53 | 0.88+-0.33 | 3.98 | Si I |
Ca I | 10 | ... | 0.65+-0.18 | 2.59 | -3.75 | 0.66+-0.18 | 2.59 | Ca I |
Sc II | 5 | ... | -0.07+-0.16 | -1.13 | -4.28 | 0.13+-0.16 | -1.13 | Sc II |
Ti I | 4 | ... | 0.41+-0.16 | 0.96 | -3.99 | 0.42+-0.16 | 0.96 | Ti I |
Ti II | 16 | ... | -0.06+-0.15 | 0.68 | -4.27 | 0.14+-0.15 | 0.68 | Ti II |
V II | 2 | ... | <0.54 | <0.26 | <-3.67 | <0.74 | <0.26 | V II |
Cr I | 4 | ... | -0.32+-0.14 | 0.92 | -4.72 | -0.31+-0.14 | 0.92 | Cr I |
Mn I | 3 | ... | -0.66+-0.15 | 0.36 | -5.07 | -0.66+-0.15 | 0.36 | Mn I |
Mn II | 3 | ... | -0.64+-0.21 | 0.57 | -4.86 | -0.45+-0.21 | 0.57 | Mn II |
Fe I | 69 | -4.41+-0.15 | ... | 3.09 | -4.41+-0.15 | ... | 3.09 | Fe I |
Fe II | 4 | -4.21+-0.16 | ... | 3.29 | -4.21+-0.16 | ... | 3.29 | Fe II |
Co I | 7 | ... | 0.29+-0.19 | 0.88 | -4.11 | 0.30+-0.19 | 0.88 | Co I |
Ni I | 10 | ... | 0.06+-0.26 | 1.87 | -4.35 | 0.06+-0.26 | 1.87 | Ni I |
Zn I | 2 | ... | <1.17 | <1.32 | <-3.24 | <1.17 | <1.32 | Zn I |
Sr II | 2 | ... | -1.95+-0.15 | -3.29 | -6.16 | -1.75+-0.15 | -3.29 | Sr II |
Y II | 6 | ... | <-0.95 | <-2.95 | <-5.16 | <-0.75 | <-2.95 | Y II |
Zr II | 3 | ... | <0.07 | <-1.56 | <-4.14 | <0.27 | <-1.56 | Zr II |
Nb II | 1 | ... | <2.55 | <-0.20 | <-1.66 | <2.75 | <-0.20 | Nb II |
Mo I | 1 | ... | <1.76 | <-0.77 | <-2.65 | <1.76 | <-0.77 | Mo I |
Tc I | 1 | ... | ... | <-0.24 | <-0.24 | <4.17 | <-0.24 | Tc I |
Ba II | 1 | ... | -1.84+-0.19 | -3.87 | -6.05 | -1.64+-0.19 | -3.87 | Ba II |
La II | 4 | ... | <0.40 | <-2.71 | <-3.81 | <0.60 | <-2.71 | La II |
Ce II | 5 | ... | <0.67 | <-1.96 | <-3.54 | <0.87 | <-1.96 | Ce II |
Pr II | 5 | ... | <1.03 | <-2.46 | <-3.18 | <1.23 | <-2.46 | Pr II |
Nd II | 5 | ... | <0.56 | <-2.23 | <-3.65 | <0.76 | <-2.23 | Nd II |
Sm II | 2 | ... | <1.20 | <-2.05 | <-3.01 | <1.40 | <-2.05 | Sm II |
Eu II | 4 | ... | <0.48 | <-3.21 | <-3.73 | <0.68 | <-3.21 | Eu II |
Gd II | 3 | ... | <1.50 | <-1.64 | <-2.71 | <1.70 | <-1.64 | Gd II |
Tb II | 2 | ... | <1.60 | <-2.31 | <-2.63 | <1.78 | <-2.31 | Tb II |
Dy II | 2 | ... | <0.80 | <-2.31 | <-3.41 | <1.00 | <-2.31 | Dy II |
Ho II | 1 | ... | <1.10 | <-2.63 | <-3.10 | <1.31 | <-2.63 | Ho II |
Er II | 3 | ... | <1.03 | <-2.26 | <-3.18 | <1.23 | <-2.26 | Er II |
Tm II | 2 | ... | <1.57 | <-2.54 | <-2.66 | <1.75 | <-2.54 | Tm II |
Yb II | 1 | ... | <0.04 | <-3.25 | <-4.17 | <0.24 | <-3.25 | Yb II |
Hf II | 2 | ... | <1.91 | <-1.45 | <-2.16 | <2.25 | <-1.45 | Hf II |
Pb I | 1 | ... | <2.60 | <0.23 | <-1.81 | <2.60 | <0.23 | Pb I |
Th II | 3 | ... | <1.66 | <-2.49 | <-2.55 | <1.86 | <-2.49 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | -249.1 |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-08-06-02:40 | 2453953.616 | MIKELCO | 41000 | 75-120 | 2100 | -249.1 |
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 | ... | -0.11 | ... | -3.81 | -0.02 | 2.43 | Na |
Mg | N/A | ... | 0.46 | ... | -3.35 | 0.44 | 4.25 | Mg |
Ca | N/A | ... | 0.58 | ... | -3.19 | 0.60 | 3.15 | Ca |
Ti | N/A | ... | 0.36 | ... | -3.36 | 0.43 | 1.59 | Ti |
Fe | N/A | -3.79 | ... | ... | -3.79 | ... | 3.71 | Fe |
Ni | N/A | ... | 0.83 | ... | -2.93 | 0.86 | 3.29 | Ni |
Position
Right Ascension : 20 20 51.17 | Declination : -39 53 30.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log