CS22952-015
HE2334-0604 in P.S.Barklem+,AAP, 439, 129, 2005
taken from 15 paper(s):
/R.Cayrel et al.(2004)/
/S.Honda et al.(2004)/
/M.Spite et al.(2005)/
/A.McWilliam et al.(1995)/
/A.McWilliam et al.(1995)/
/S.Honda et al.(2004)/
/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)/
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 : 2.1 |
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 | 8 | -3.43+-0.08 | 0.00+-0.08 | 4.15+-0.08 | -3.45+-0.08 | 0.00+-0.08 | 4.15+-0.08 | Mg I |
Al I | 2 | -3.89 | -0.46 | 2.58 | -3.87 | -0.42 | 2.58 | Al I |
Si I | 1 | -3.10 | 0.33 | 4.45 | -3.06 | 0.39 | 4.45 | Si I |
K I | 1 | -2.94 | 0.49 | 2.18 | -2.85 | 0.60 | 2.18 | K I |
Ca I | 16 | -3.29+-0.14 | 0.14+-0.14 | 3.07+-0.14 | -3.27+-0.14 | 0.18+-0.14 | 3.07+-0.14 | Ca I |
Sc II | 7 | -3.54+-0.05 | -0.11+-0.05 | -0.37+-0.05 | -3.52+-0.05 | -0.07+-0.05 | -0.37+-0.05 | Sc II |
Ti I | 14 | -3.33+-0.09 | 0.10+-0.09 | 1.69+-0.09 | -3.26+-0.09 | 0.19+-0.09 | 1.69+-0.09 | Ti I |
Ti II | 31 | -3.43+-0.11 | 0.00+-0.11 | 1.59+-0.11 | -3.36+-0.11 | 0.09+-0.11 | 1.59+-0.11 | Ti II |
Cr I | 7 | -3.89+-0.15 | -0.46+-0.15 | 1.78+-0.15 | -3.86+-0.15 | -0.41+-0.15 | 1.78+-0.15 | Cr I |
Mn I | 3 | -3.76+-0.16 | -0.33+-0.16 | 1.63+-0.16 | -3.80+-0.16 | -0.35+-0.16 | 1.63+-0.16 | Mn I |
Fe I | 147 | -3.45+-0.14 | -0.02+-0.14 | 4.05+-0.14 | -3.45+-0.14 | -0.02+-0.14 | 4.05+-0.14 | Fe I |
Fe II | 11 | -3.41+-0.10 | 0.02+-0.10 | 4.09+-0.10 | -3.41+-0.10 | 0.02+-0.10 | 4.09+-0.10 | Fe II |
Co I | 4 | -3.30+-0.10 | 0.13+-0.10 | 1.62+-0.10 | -3.37+-0.10 | 0.08+-0.10 | 1.62+-0.10 | Co I |
Ni I | 3 | -3.55+-0.10 | -0.12+-0.10 | 2.70+-0.10 | -3.52+-0.10 | -0.07+-0.10 | 2.70+-0.10 | Ni I |
Zn I | 1 | -3.18 | 0.25 | 1.42 | -3.14 | 0.31 | 1.42 | Zn I |
Binary Parameters
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 | 150 | 10200 | N/A |
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium
Stellar Parameters
Teff : 4850 | log g : 1.5 | vturb : 1.5 |
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 | ... | -0.22 | 5.4 | -3.03 | -0.10 | 5.4 | CH |
Mg I | 5 | ... | -0.19+-0.21 | 4.45+-0.21 | -3.15+-0.21 | -0.22+-0.21 | 4.45+-0.21 | Mg I |
Al I | 1 | ... | -0.68+-0.19 | 2.85+-0.19 | -3.60+-0.19 | -0.67+-0.19 | 2.85+-0.19 | Al I |
Si I | 1 | ... | 0.39+-0.19 | 5+-0.19 | -2.51+-0.19 | 0.42+-0.19 | 5+-0.19 | Si I |
Ca I | 2 | ... | 0.03+-0.16 | 3.45+-0.16 | -2.89+-0.16 | 0.04+-0.16 | 3.45+-0.16 | Ca I |
Sc II | 2 | ... | -0.36+-0.06 | -0.13+-0.06 | -3.28+-0.06 | -0.35+-0.06 | -0.13+-0.06 | Sc II |
Ti | 13 | ... | -0.12+-0.06 | 1.96+-0.06 | -2.99+-0.06 | -0.06+-0.06 | 1.96+-0.06 | Ti |
V | 1 | ... | -0.03+-0.19 | 1.03+-0.19 | -2.90+-0.19 | 0.03+-0.19 | 1.03+-0.19 | V |
Mn I | 3 | ... | -0.34+-0.39 | 2.11+-0.39 | -3.32+-0.39 | -0.39+-0.39 | 2.11+-0.39 | Mn I |
Fe | N/A | -2.94+-0.26 | ... | 4.57+-0.26 | -2.93+-0.26 | ... | 4.57+-0.26 | Fe |
Co I | 2 | ... | 0.06+-0.19 | 2.04+-0.19 | -2.95+-0.19 | -0.02+-0.19 | 2.04+-0.19 | Co I |
Ni I | 2 | ... | -0.11+-0.19 | 3.2+-0.19 | -3.02+-0.19 | -0.09+-0.19 | 3.2+-0.19 | Ni I |
Sr II | 2 | ... | -0.71+-0.19 | -0.73+-0.19 | -3.60+-0.19 | -0.67+-0.19 | -0.73+-0.19 | Sr II |
Ba II | 2 | ... | -1.77+-0.19 | -2.49+-0.19 | -4.67+-0.19 | -1.74+-0.19 | -2.49+-0.19 | Ba II |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-11-11 | N/A | SUBARUHDS | 50000 | 59 | 9000 | -20.07+-0.71 |
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 : 2.1 |
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 | ... | ... | <-0.40 | <-3.66 | <-0.23 | <-0.40 | Li I |
C | N/A | -4.02+-0.08 | ... | ... | -3.93+-0.08 | -0.50+-0.08 | 4.50+-0.08 | C |
N | N/A | -2.12 | ... | ... | -2.03 | 1.40 | 5.80 | N |
Fe | N/A | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 4720 | log g : 0.90+-0.27 | vturb : 2.55+-0.08 |
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 | ... | <-3.35 | <-0.14 | <5.08 | C |
Na | N/A | ... | -0.18 | ... | -3.47 | -0.26 | 2.77 | Na |
Mg | N/A | ... | -0.33 | ... | -3.73 | -0.52 | 3.87 | Mg |
Ca | N/A | ... | 0.34 | ... | -3.02 | 0.19 | 3.32 | Ca |
Fe I | N/A | -3.38 | ... | ... | -3.21 | ... | 4.29 | Fe I |
Fe II | N/A | -3.42 | ... | ... | -3.25 | ... | 4.25 | Fe II |
Ni | N/A | ... | 0.01 | ... | -3.34 | -0.13 | 2.88 | Ni |
Sr | N/A | ... | -0.94 | ... | -4.29 | -1.08 | -1.42 | Sr |
Ba | N/A | ... | -1.45 | ... | -4.88 | -1.67 | -2.70 | Ba |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 |
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. I. Observational Data
Binary Parameters
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-11-11 | N/A | SUBARUHDS | 50000 | 59 | 9000 | -20.07+-0.71 |
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 : 2.1 |
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 | -4.02+-0.08 | ... | ... | -3.93+-0.08 | -0.50+-0.08 | 4.50+-0.08 | C |
N | N/A | -2.12+-0.10 | ... | ... | -2.03+-0.10 | 1.40+-0.10 | 5.80+-0.10 | N |
Fe | N/A | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 2.1 |
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 | -2.92 | +0.51 | 3.33 | -2.91 | 0.52 | 3.33 | Na |
Fe | N/A | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 4800 | log g : 1.3 | vturb : 2.1 |
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 | -3.42 | 0.01 | 3.05 | -3.40 | 0.03 | 3.05 | Al |
Fe | N/A | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 4800 | log g : 1.3 | vturb : 2.1 |
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 | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Ba | 1 | ... | ... | -2.63 | -4.81 | -1.38 | -2.63 | Ba |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 2.1 |
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 | ... | ... | 4.20 | -3.40 | 0.03 | 4.20 | Mg |
K | N/A | ... | ... | 2.15 | -2.88 | 0.55 | 2.15 | K |
Fe | N/A | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 4800 | log g : 1.3 | vturb : 2.1 |
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 | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Sr | 2 | ... | -0.99 | ... | -4.37 | -0.94 | -1.50 | Sr |
Y | 7 | ... | -0.90 | ... | -4.30 | -0.87 | -2.09 | Y |
Zr | 3 | ... | -0.52 | ... | -3.93 | -0.50 | -1.35 | Zr |
Ba | 3 | ... | -1.33 | ... | -4.81 | -1.38 | -2.63 | Ba |
La | N/A | ... | <-0.54 | ... | <-3.90 | <-0.47 | <-2.80 | La |
Ce | N/A | ... | <+0.05 | ... | <-3.38 | <0.05 | <-1.80 | Ce |
Pr | N/A | ... | <+0.07 | ... | <-3.37 | <0.06 | <-2.65 | Pr |
Nd | N/A | ... | <-0.37 | ... | <-3.72 | <-0.29 | <-2.30 | Nd |
Sm | N/A | ... | <-0.37 | ... | <-3.75 | <-0.32 | <-2.79 | Sm |
Eu | N/A | ... | <-0.28 | ... | <-3.72 | <-0.29 | <-3.20 | Eu |
Gd | N/A | ... | <+0.01 | ... | <-3.37 | <0.06 | <-2.30 | Gd |
Dy | N/A | ... | <-0.71 | ... | <-4.10 | <-0.67 | <-3.00 | Dy |
Ho | N/A | ... | <-0.13 | ... | <-3.77 | <-0.34 | <-3.30 | Ho |
Er | N/A | ... | <+0.00 | ... | <-3.42 | <0.01 | <-2.50 | Er |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 2.1 |
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 | -3.07 | 0.36 | ... | -3.05 | 0.38 | 3.29 | Ca |
Fe | N/A | -3.43 | ... | ... | -3.43 | ... | 4.07 | Fe |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | 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 : 4500+-33 | log g : 0.55+-0.13 | 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 | ... | ... | <0.15 | <-3.11 | <0.76 | <0.15 | Li I |
CH | 1 | ... | -0.84+-0.25 | 3.91 | -4.52 | -0.65+-0.25 | 3.91 | CH |
NH | 1 | ... | 0.95+-0.36 | 5.10 | -2.73 | 1.14+-0.36 | 5.10 | NH |
O I | 3 | ... | <1.84 | <6.66 | <-2.03 | <1.84 | <6.66 | O I |
Mg I | 8 | ... | 0.30+-0.17 | 4.03 | -3.57 | 0.30+-0.17 | 4.03 | Mg I |
Al I | 2 | ... | -0.18+-0.30 | 2.40 | -4.05 | -0.18+-0.30 | 2.40 | Al I |
Si I | 2 | ... | 0.83+-0.22 | 4.47 | -3.04 | 0.83+-0.22 | 4.47 | Si I |
Ca I | 11 | ... | 0.34+-0.18 | 2.81 | -3.53 | 0.34+-0.18 | 2.81 | Ca I |
Sc II | 5 | ... | -0.26+-0.15 | -0.79 | -3.94 | -0.07+-0.15 | -0.79 | Sc II |
Ti I | 8 | ... | 0.00+-0.15 | 1.08 | -3.87 | 0.00+-0.15 | 1.08 | Ti I |
Ti II | 25 | ... | -0.08+-0.15 | 1.19 | -3.76 | 0.11+-0.15 | 1.19 | Ti II |
V II | 1 | ... | -0.29+-0.29 | -0.04 | -3.97 | -0.10+-0.29 | -0.04 | V II |
Cr I | 5 | ... | -0.29+-0.15 | 1.48 | -4.16 | -0.29+-0.15 | 1.48 | Cr I |
Mn I | 4 | ... | -0.45+-0.17 | 1.11 | -4.32 | -0.45+-0.17 | 1.11 | Mn I |
Fe I | 100 | -3.87+-0.15 | ... | 3.63 | -3.87+-0.15 | ... | 3.63 | Fe I |
Fe II | 10 | -3.68+-0.16 | ... | 3.82 | -3.68+-0.16 | ... | 3.82 | Fe II |
Co I | 7 | ... | -0.12+-0.19 | 1.00 | -3.99 | -0.12+-0.19 | 1.00 | Co I |
Ni I | 8 | ... | -0.14+-0.23 | 2.21 | -4.01 | -0.14+-0.23 | 2.21 | Ni I |
Zn I | 2 | ... | 0.46+-0.19 | 1.15 | -3.41 | 0.46+-0.19 | 1.15 | Zn I |
Rb I | 1 | ... | <3.09 | <1.74 | <-0.62 | <3.25 | <1.74 | Rb I |
Sr II | 2 | ... | -0.84+-0.23 | -1.65 | -4.52 | -0.65+-0.23 | -1.65 | Sr II |
Y II | 1 | ... | -1.46+-0.23 | -2.93 | -5.14 | -1.27+-0.23 | -2.93 | Y II |
Nb II | 1 | ... | <1.91 | <-0.31 | <-1.77 | <2.10 | <-0.31 | Nb II |
Mo I | 1 | ... | <1.14 | <-0.85 | <-2.73 | <1.14 | <-0.85 | Mo I |
Tc I | 1 | ... | ... | <-0.63 | <-0.63 | <3.24 | <-0.63 | Tc I |
Sn I | 1 | ... | <2.55 | <0.75 | <-1.32 | <2.55 | <0.75 | Sn I |
Ba II | 1 | ... | -1.69+-0.15 | -3.19 | -5.37 | -1.50+-0.15 | -3.19 | Ba II |
Ce II | 5 | ... | <-0.10 | <-2.20 | <-3.78 | <0.09 | <-2.20 | Ce II |
Pr II | 5 | ... | <0.52 | <-2.44 | <-3.16 | <0.71 | <-2.44 | Pr II |
Nd II | 5 | ... | <-0.18 | <-2.44 | <-3.86 | <0.01 | <-2.44 | Nd II |
Sm II | 2 | ... | <0.49 | <-2.23 | <-3.19 | <0.68 | <-2.23 | Sm II |
Eu II | 4 | ... | <-0.28 | <-3.44 | <-3.96 | <-0.09 | <-3.44 | Eu II |
Gd II | 3 | ... | <0.84 | <-1.77 | <-2.84 | <1.03 | <-1.77 | Gd II |
Tb II | 4 | ... | <0.84 | <-2.54 | <-2.86 | <1.01 | <-2.54 | Tb II |
Dy II | 3 | ... | <-0.08 | <-2.66 | <-3.76 | <0.11 | <-2.66 | Dy II |
Ho II | 2 | ... | <0.40 | <-2.80 | <-3.27 | <0.60 | <-2.80 | Ho II |
Er II | 3 | ... | <0.33 | <-2.43 | <-3.35 | <0.52 | <-2.43 | Er II |
Tm II | 2 | ... | <0.72 | <-2.86 | <-2.98 | <0.89 | <-2.86 | Tm II |
Yb II | 1 | ... | <-0.57 | <-3.33 | <-4.25 | <-0.38 | <-3.33 | Yb II |
Hf II | 1 | ... | <1.33 | <-1.50 | <-2.21 | <1.66 | <-1.50 | Hf II |
Ir I | 1 | ... | <1.30 | <-1.19 | <-2.57 | <1.30 | <-1.19 | Ir I |
Pb I | 1 | ... | <1.99 | <0.16 | <-1.88 | <1.99 | <0.16 | Pb I |
Th II | 3 | ... | <0.91 | <-2.71 | <-2.77 | <1.10 | <-2.71 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | -17.9 |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-08-04-09:06 | 2453951.884 | MIKELCO | 41000 | 70-120 | 1800 | -17.9 |
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 |
Mg | N/A | ... | -0.18 | ... | -3.60 | -0.20 | 4.00 | Mg |
Ca | N/A | ... | 0.34 | ... | -3.04 | 0.36 | 3.30 | Ca |
Ti | N/A | ... | 0.08 | ... | -3.25 | 0.15 | 1.70 | Ti |
Fe | N/A | -3.4 | ... | ... | -3.40 | ... | 4.10 | Fe |
Ni | N/A | ... | 0.01 | ... | -3.36 | 0.04 | 2.86 | Ni |
Ba | N/A | ... | -1.57 | ... | -5.02 | -1.62 | -2.84 | Ba |
Position
Right Ascension : 23 37 28.69 | Declination : -05 47 56.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log