CD-38_245
HIP3635 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 16 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)/
/B.W.Carney et al.(2003)/
/S.M.Andrievsky et al.(2008)/
/S.M.Andrievsky et al.(2009)/
/S.M.Andrievsky et al.(2010)/
/P.Francois et al.(2007)/
/J.K.Hollek et al.(2011)/
/M.Spite et al.(2012)/
/I.U.Roederer et al.(2014)/
EXTREMELY METAL-POOR STARS. VIII. HIGH-RESOLUTION, HIGH SIGNAL-TO-NOISE RATIO ANALYSIS OF FIVE STARS WITH [Fe/H]<=-3.5
Stellar Parameters
Teff : 4850 | log g : 1.8 | 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 |
CH | N/A | ... | <0.00+-0.20 | ... | <-3.74+-0.20 | <0.07+-0.20 | <4.69+-0.20 | CH |
Mg I | 5 | ... | 0.45+-0.09 | ... | -3.55+-0.09 | 0.26+-0.09 | 4.05+-0.09 | Mg I |
Al I | 1 | ... | -0.77+-0.23 | ... | -4.73+-0.23 | -0.92+-0.23 | 1.72+-0.23 | Al I |
Si I | 2 | ... | 0.30+-0.21 | ... | -3.64+-0.21 | 0.17+-0.21 | 3.87+-0.21 | Si I |
Ca I | 6 | ... | 0.14+-0.11 | ... | -3.82+-0.11 | -0.01+-0.11 | 2.52+-0.11 | Ca I |
Sc II | 6 | ... | 0.08+-0.16 | ... | -3.96+-0.16 | -0.15+-0.16 | -0.81+-0.16 | Sc II |
Ti I | 2 | ... | 0.28+-0.14 | ... | -3.66+-0.14 | 0.15+-0.14 | 1.29+-0.14 | Ti I |
Ti II | 27 | ... | 0.37+-0.15 | ... | -3.57+-0.15 | 0.24+-0.15 | 1.38+-0.15 | Ti II |
V II | 1 | ... | <0.52+-0.19 | ... | <-3.39+-0.19 | <0.42+-0.19 | <0.54+-0.19 | V II |
Cr I | 3 | ... | -0.65+-0.11 | ... | -4.60+-0.11 | -0.79+-0.11 | 1.04+-0.11 | Cr I |
Mn I | 3 | ... | -1.05+-0.14 | ... | -5.07+-0.14 | -1.26+-0.14 | 0.36+-0.14 | Mn I |
Fe I | 92 | -3.98+-0.15 | ... | ... | -3.81+-0.15 | ... | 3.69+-0.15 | Fe I |
Fe II | 2 | -3.98+-0.25 | ... | ... | -3.81+-0.25 | ... | 3.69+-0.25 | Fe II |
Co I | 4 | ... | 0.49+-0.12 | ... | -3.56+-0.12 | 0.25+-0.12 | 1.43+-0.12 | Co I |
Ni I | 5 | ... | -0.12+-0.09 | ... | -4.07+-0.09 | -0.26+-0.09 | 2.15+-0.09 | Ni I |
Sr II | 2 | ... | -0.70+-0.16 | ... | -4.65+-0.16 | -0.84+-0.16 | -1.78+-0.16 | Sr II |
Y II | 1 | ... | <-1.42+-0.15 | ... | <-5.37+-0.15 | <-1.56+-0.15 | <-3.16+-0.15 | Y II |
Ba II | 1 | ... | -0.86+-0.23 | ... | -4.89+-0.23 | -1.08+-0.23 | -2.71+-0.23 | Ba II |
Eu II | 1 | ... | <0.82+-0.18 | ... | <-3.17+-0.18 | <0.64+-0.18 | <-2.65+-0.18 | Eu II |
Binary Parameters
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 | 45.9+-1.1 |
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Stellar Parameters
Teff : 4800 | log g : 1.5 | vturb : 2.2 |
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 |
CH | N/A | <-4.52 | <-0.33 | <4.00 | <-4.43 | <-0.23 | <4.00 | CH |
Na I | 2 | -4.25 | -0.06 | 2.08 | -4.16 | 0.04 | 2.08 | Na I |
Mg I | 6 | -3.99+-0.08 | 0.20+-0.08 | 3.59+-0.08 | -4.01+-0.08 | 0.19+-0.08 | 3.59+-0.08 | Mg I |
Al I | 2 | -4.86 | -0.67 | 1.61 | -4.84 | -0.64 | 1.61 | Al I |
Si I | 1 | -3.99 | 0.20 | 3.56 | -3.95 | 0.25 | 3.56 | Si I |
Ca I | 8 | -3.99+-0.17 | 0.20+-0.17 | 2.37+-0.17 | -3.97+-0.17 | 0.23+-0.17 | 2.37+-0.17 | Ca I |
Sc II | 2 | -4.15 | 0.04 | -0.98 | -4.13 | 0.07 | -0.98 | Sc II |
Ti I | 5 | -3.82+-0.04 | 0.37+-0.04 | 1.20+-0.04 | -3.75+-0.04 | 0.45+-0.04 | 1.20+-0.04 | Ti I |
Ti II | 24 | -3.94+-0.11 | 0.25+-0.11 | 1.08+-0.11 | -3.87+-0.11 | 0.33+-0.11 | 1.08+-0.11 | Ti II |
Cr I | 5 | -4.63+-0.12 | -0.44+-0.12 | 1.04+-0.12 | -4.60+-0.12 | -0.40+-0.12 | 1.04+-0.12 | Cr I |
Mn I | 3 | -4.78+-0.03 | -0.60+-0.03 | 0.61+-0.03 | -4.82+-0.03 | -0.62+-0.03 | 0.61+-0.03 | Mn I |
Fe I | 95 | -4.20+-0.20 | -0.01+-0.20 | 3.30+-0.20 | -4.20+-0.20 | -0.01+-0.20 | 3.30+-0.20 | Fe I |
Fe II | 7 | -4.17+-0.13 | 0.02+-0.13 | 3.33+-0.13 | -4.17+-0.13 | 0.02+-0.13 | 3.33+-0.13 | Fe II |
Co I | 3 | -3.82+-0.08 | 0.37+-0.08 | 1.10+-0.08 | -3.89+-0.08 | 0.31+-0.08 | 1.10+-0.08 | Co I |
Ni I | 2 | -4.37 | -0.19 | 1.88 | -4.34 | -0.14 | 1.88 | Ni I |
Zn I | 1 | -3.50 | 0.69 | 1.10 | -3.46 | 0.74 | 1.10 | Zn I |
Binary Parameters
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-01 | N/A | VLT | 47000 | 200 | 14400 | 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 : 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 |
Na I | 2 | -4.14+-0.05 | ... | ... | -4.05+-0.05 | 0.02+-0.05 | 2.19+-0.05 | Na I |
Mg I | 3 | -3.73+-0.05 | ... | ... | -3.75+-0.05 | 0.32+-0.05 | 3.85+-0.05 | Mg I |
Al I | 2 | -4.80+-0.00 | ... | ... | -4.78+-0.00 | -0.71+-0.00 | 1.67+-0.00 | Al I |
Si I | 1 | -3.90 | ... | ... | -3.86 | 0.21 | 3.65 | Si I |
Ca I | 7 | -3.80+-0.13 | ... | ... | -3.78+-0.13 | 0.29+-0.13 | 2.56+-0.13 | Ca I |
Sc II | 2 | -3.99+-0.00 | ... | ... | -3.97+-0.00 | 0.10+-0.00 | -0.82+-0.00 | Sc II |
Ti I | 4 | -3.74+-0.05 | ... | ... | -3.67+-0.05 | 0.40+-0.05 | 1.28+-0.05 | Ti I |
Cr I | 5 | -4.42+-0.11 | ... | ... | -4.39+-0.11 | -0.32+-0.11 | 1.25+-0.11 | Cr I |
Mn I | 3 | -5.08+-0.03 | ... | ... | -5.12+-0.03 | -1.05+-0.03 | 0.31+-0.03 | Mn I |
Fe I | 77 | -4.07+-0.15 | ... | ... | -4.07+-0.15 | ... | 3.43+-0.15 | Fe I |
Fe II | 6 | -3.99+-0.13 | ... | ... | -3.99+-0.13 | ... | 3.51+-0.13 | Fe II |
Co I | 3 | -3.67+-0.08 | ... | ... | -3.74+-0.08 | 0.33+-0.08 | 1.25+-0.08 | Co I |
Ni I | 2 | -4.20+-0.00 | ... | ... | -4.17+-0.00 | -0.10+-0.00 | 2.05+-0.00 | Ni I |
Sr II | 2 | -4.72+-0.08 | ... | ... | -4.67+-0.08 | -0.60+-0.08 | -1.80+-0.08 | Sr II |
Y II | 2 | -4.61+-0.03 | ... | ... | -4.58+-0.03 | -0.51+-0.03 | -2.37+-0.03 | Y II |
Ba II | 1 | -4.73 | ... | ... | -4.78 | -0.71 | -2.60 | Ba II |
Eu II | 1 | <-3.51 | ... | ... | <-3.52 | <0.55 | <-3.00 | Eu II |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 | 45000 | 150 | 7200 | 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 : 4800 | log g : 1.5 | vturb : 2.2 |
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 |
Li I | N/A | ... | ... | <-0.40 | <-3.66 | <0.53 | <-0.40 | Li I |
C | N/A | <-4.52 | ... | ... | <-4.43 | <-0.24 | <4.00 | C |
N | N/A | -3.12 | ... | ... | -3.03 | 1.16 | 4.80 | N |
Fe | N/A | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 |
A Spectroscopic Analysis of 33 of the Most Metal-Poor Stars.I.
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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.
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 | ... | <-3.98 | <-0.14 | <4.45 | C |
Na | N/A | ... | -0.10 | ... | -4.02 | -0.18 | 2.22 | Na |
Mg | N/A | ... | 0.38 | ... | -3.65 | 0.19 | 3.95 | Mg |
Ca | N/A | ... | 0.58 | ... | -3.41 | 0.43 | 2.93 | Ca |
Fe I | N/A | -4.01 | ... | ... | -3.84 | ... | 3.66 | Fe I |
Fe II | N/A | -4.00 | ... | ... | -3.83 | ... | 3.67 | Fe II |
Ni | N/A | ... | -0.12 | ... | -4.10 | -0.26 | 2.12 | Ni |
Sr | N/A | ... | -0.61 | ... | -4.59 | -0.75 | -1.72 | Sr |
Ba | N/A | ... | 0.02 | ... | -4.04 | -0.20 | -1.86 | Ba |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 : 1.5 | vturb : 2.2 |
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 |
C | N/A | <-4.52 | ... | ... | <-4.43 | <-0.24 | <4.00 | C |
N | N/A | -3.12+-0.20 | ... | ... | -3.03+-0.20 | 1.16+-0.20 | 4.80+-0.20 | N |
Fe | N/A | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 : 1.5 | vturb : 2.2 |
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 |
Na | N/A | -4.10 | +0.09 | 2.15 | -4.09 | 0.10 | 2.15 | Na |
Fe | N/A | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 |
Spectroscopic Binaries, Velocity Jitter, and Rotation in Field Metal-poor Red Giant and Red Horizontal-Branch 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 |
Fe | N/A | -4.00 | ... | ... | -4.00 | ... | 3.50 | Fe |
Binary Parameters
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 | 2446005.68340 | MMT | N/A | N/A | N/A | 48.04+-1.68 |
N/A | 2446397.66162 | MMT | N/A | N/A | N/A | 46.29+-0.67 |
N/A | 2446725.73743 | MMT | N/A | N/A | N/A | 46.57+-0.97 |
N/A | 2447047.89309 | TILLINGHAST | N/A | N/A | N/A | 47.17+-0.74 |
N/A | 2447429.84452 | TILLINGHAST | N/A | N/A | N/A | 46.48+-1.03 |
N/A | 2449355.60411 | MMT | N/A | N/A | N/A | 46.46+-0.62 |
N/A | 2450799.69885 | MMT | N/A | N/A | N/A | 43.97+-1.17 |
NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4800 | log g : 1.5 | vturb : 2.2 |
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 |
Al | N/A | -4.12 | 0.07 | 2.35 | -4.10 | 0.09 | 2.35 | Al |
Fe | N/A | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 |
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 : 1.5 | vturb : 2.2 |
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 | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Ba | 1 | ... | ... | -2.82 | -5.00 | -0.81 | -2.82 | Ba |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 : 1.5 | vturb : 2.2 |
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 |
Mg | N/A | ... | ... | 3.66 | -3.94 | 0.25 | 3.66 | Mg |
Fe | N/A | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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. VIII. Enrichment of the neutron-capture elements in the early Galaxy
Stellar Parameters
Teff : 4800 | log g : 1.5 | vturb : 2.2 |
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 | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Sr | 3 | ... | -0.71 | ... | -4.85 | -0.66 | -1.98 | Sr |
Y | 2 | ... | -0.45 | ... | -4.61 | -0.42 | -2.40 | Y |
Zr | N/A | ... | <-0.11 | ... | <-4.28 | <-0.09 | <-1.70 | Zr |
Ba | 2 | ... | -0.76 | ... | -5.00 | -0.81 | -2.82 | Ba |
La | N/A | ... | <+0.02 | ... | <-4.10 | <0.09 | <-3.00 | La |
Ce | N/A | ... | <+0.71 | ... | <-3.48 | <0.71 | <-1.90 | Ce |
Pr | N/A | ... | <+0.83 | ... | <-3.37 | <0.82 | <-2.65 | Pr |
Nd | N/A | ... | <+0.19 | ... | <-3.92 | <0.27 | <-2.50 | Nd |
Sm | N/A | ... | <+1.28 | ... | <-2.86 | <1.33 | <-1.90 | Sm |
Eu | N/A | ... | <+0.38 | ... | <-3.82 | <0.37 | <-3.30 | Eu |
Gd | N/A | ... | <+0.77 | ... | <-3.37 | <0.82 | <-2.30 | Gd |
Dy | N/A | ... | <+0.95 | ... | <-3.20 | <0.99 | <-2.10 | Dy |
Ho | N/A | ... | <+0.53 | ... | <-3.87 | <0.32 | <-3.40 | Ho |
Er | N/A | ... | <+0.86 | ... | <-3.32 | <0.87 | <-2.40 | Er |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 |
The Chemical Abundances of Stars in the Halo (CASH) Project. II. A Sample of 14 Extremely Metal-poor Stars
Stellar Parameters
Teff : 4650 | log g : 0.95 | vturb : 2.15 |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2009-07-27 | N/A | MIKELCO | 35000 | 65 | 250 | 47.1 |
NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
Stellar Parameters
Teff : 4800 | log g : 1.5 | vturb : 2.2 |
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 |
Ca | N/A | -3.64 | 0.55 | ... | -3.62 | 0.57 | 2.72 | Ca |
Fe | N/A | -4.19 | ... | ... | -4.19 | ... | 3.31 | Fe |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | 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 |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 4520+-34 | log g : 0.65+-0.13 | vturb : 1.8+-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 | ... | ... | <0.01 | <-3.25 | <1.34 | <0.01 | Li I |
CH | 1 | ... | <-0.29 | <3.65 | <-4.78 | <-0.19 | <3.65 | CH |
NH | 1 | ... | <1.56 | <4.90 | <-2.93 | <1.66 | <4.90 | NH |
O I | 4 | ... | <2.26 | <6.36 | <-2.33 | <2.26 | <6.36 | O I |
Mg I | 7 | ... | 0.66+-0.18 | 3.67 | -3.93 | 0.66+-0.18 | 3.67 | Mg I |
Al I | 2 | ... | -0.63+-0.17 | 1.23 | -5.22 | -0.63+-0.17 | 1.23 | Al I |
Si I | 1 | ... | 0.53+-0.32 | 3.45 | -4.06 | 0.53+-0.32 | 3.45 | Si I |
Ca I | 5 | ... | 0.48+-0.19 | 2.23 | -4.11 | 0.48+-0.19 | 2.23 | Ca I |
Sc II | 6 | ... | -0.22+-0.17 | -1.57 | -4.72 | -0.13+-0.17 | -1.57 | Sc II |
Ti I | 4 | ... | 0.49+-0.19 | 0.85 | -4.10 | 0.49+-0.19 | 0.85 | Ti I |
Ti II | 18 | ... | 0.22+-0.15 | 0.67 | -4.28 | 0.31+-0.15 | 0.67 | Ti II |
V II | 2 | ... | <0.38 | <-0.19 | <-4.12 | <0.47 | <-0.19 | V II |
Cr I | 4 | ... | -0.44+-0.15 | 0.61 | -5.03 | -0.44+-0.15 | 0.61 | Cr I |
Mn I | 3 | ... | -0.90+-0.16 | -0.06 | -5.49 | -0.90+-0.16 | -0.06 | Mn I |
Mn II | 1 | ... | -0.57+-0.21 | 0.36 | -5.07 | -0.48+-0.21 | 0.36 | Mn II |
Fe I | 71 | -4.59+-0.16 | ... | 2.91 | -4.59+-0.16 | ... | 2.91 | Fe I |
Fe II | 3 | -4.50+-0.17 | ... | 3.00 | -4.50+-0.17 | ... | 3.00 | Fe II |
Co I | 7 | ... | 0.18+-0.20 | 0.58 | -4.41 | 0.18+-0.20 | 0.58 | Co I |
Ni I | 7 | ... | -0.11+-0.22 | 1.52 | -4.70 | -0.11+-0.22 | 1.52 | Ni I |
Zn I | 2 | ... | 1.08+-0.21 | 1.05 | -3.51 | 1.08+-0.21 | 1.05 | Zn I |
Rb I | 1 | ... | <3.50 | <1.43 | <-0.93 | <3.66 | <1.43 | Rb I |
Sr II | 2 | ... | -0.73+-0.15 | -2.35 | -5.22 | -0.63+-0.15 | -2.35 | Sr II |
Y II | 6 | ... | <-0.77 | <-3.06 | <-5.27 | <-0.68 | <-3.06 | Y II |
Zr II | 3 | ... | <0.09 | <-1.83 | <-4.41 | <0.18 | <-1.83 | Zr II |
Nb II | 1 | ... | <2.59 | <-0.45 | <-1.91 | <2.68 | <-0.45 | Nb II |
Mo I | 1 | ... | <1.75 | <-0.96 | <-2.84 | <1.75 | <-0.96 | Mo I |
Tc I | 1 | ... | ... | <-0.81 | <-0.81 | <3.78 | <-0.81 | Tc I |
Sn I | 1 | ... | <2.95 | <0.43 | <-1.64 | <2.95 | <0.43 | Sn I |
Ba II | 2 | ... | -1.10+-0.17 | -3.41 | -5.59 | -1.00+-0.17 | -3.41 | Ba II |
Ce II | 5 | ... | <0.53 | <-2.39 | <-3.97 | <0.62 | <-2.39 | Ce II |
Pr II | 5 | ... | <1.14 | <-2.64 | <-3.36 | <1.23 | <-2.64 | Pr II |
Nd II | 5 | ... | <0.60 | <-2.48 | <-3.90 | <0.69 | <-2.48 | Nd II |
Sm II | 2 | ... | <1.22 | <-2.32 | <-3.28 | <1.31 | <-2.32 | Sm II |
Eu II | 1 | ... | <0.60 | <-3.38 | <-3.90 | <0.69 | <-3.38 | Eu II |
Gd II | 3 | ... | <1.51 | <-1.92 | <-2.99 | <1.60 | <-1.92 | Gd II |
Tb II | 3 | ... | <1.56 | <-2.64 | <-2.96 | <1.63 | <-2.64 | Tb II |
Dy II | 3 | ... | <0.74 | <-2.66 | <-3.76 | <0.83 | <-2.66 | Dy II |
Er II | 3 | ... | <1.00 | <-2.58 | <-3.50 | <1.09 | <-2.58 | Er II |
Tm II | 2 | ... | <1.46 | <-2.94 | <-3.06 | <1.53 | <-2.94 | Tm II |
Yb II | 1 | ... | <0.21 | <-3.37 | <-4.29 | <0.30 | <-3.37 | Yb II |
Hf II | 2 | ... | <1.97 | <-1.68 | <-2.39 | <2.20 | <-1.68 | Hf II |
Ir I | 1 | ... | <1.96 | <-1.25 | <-2.63 | <1.96 | <-1.25 | Ir I |
Pb I | 1 | ... | <2.34 | <-0.21 | <-2.25 | <2.34 | <-0.21 | Pb I |
Th II | 3 | ... | <1.70 | <-2.74 | <-2.80 | <1.79 | <-2.74 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | 46.1 |
Position
Right Ascension : 00 46 36.10 | Declination : -37 39 33.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-06-24-10:33 | 2452814.94 | MIKEBAADE | 41000 | 120-255 | 800 | 46.1 |
2004-09-24-07:22 | 2453272.811 | MIKELCO | 41000 | 120-255 | 480 | 46.2 |