CS22968-014
HE0305-5442 in J.G.Cohen+,ApJ, 778, 56, 2013
taken from 14 paper(s):
/R.Cayrel et al.(2004)/
/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)/
/J.A.Johnson 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 : 4850 | log g : 1.7 | 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 | -3.26 | 0.30 | 5.26 | -3.17 | 0.40 | 5.26 | CH |
[O I] | N/A | -2.66 | 0.90 | 6.11 | -2.58 | 0.99 | 6.11 | [O I] |
Na I | 2 | -3.92 | -0.37 | 2.41 | -3.83 | -0.26 | 2.41 | Na I |
Mg I | 8 | -3.36+-0.13 | 0.19+-0.13 | 4.22+-0.13 | -3.38+-0.13 | 0.19+-0.13 | 4.22+-0.13 | Mg I |
Al I | 2 | -4.34 | -0.79 | 2.13 | -4.32 | -0.75 | 2.13 | Al I |
Si I | 1 | -3.35 | 0.21 | 4.20 | -3.31 | 0.26 | 4.20 | Si I |
K I | 2 | -3.34 | 0.22 | 1.78 | -3.25 | 0.32 | 1.78 | K I |
Ca I | 17 | -3.53+-0.17 | 0.02+-0.17 | 2.83+-0.17 | -3.51+-0.17 | 0.06+-0.17 | 2.83+-0.17 | Ca I |
Sc II | 7 | -3.52+-0.07 | 0.03+-0.07 | -0.35+-0.07 | -3.50+-0.07 | 0.07+-0.07 | -0.35+-0.07 | Sc II |
Ti I | 14 | -3.45+-0.12 | 0.11+-0.12 | 1.57+-0.12 | -3.38+-0.12 | 0.19+-0.12 | 1.57+-0.12 | Ti I |
Ti II | 28 | -3.55+-0.12 | 0.00+-0.12 | 1.47+-0.12 | -3.48+-0.12 | 0.09+-0.12 | 1.47+-0.12 | Ti II |
Cr I | 7 | -4.01+-0.16 | -0.46+-0.16 | 1.66+-0.16 | -3.98+-0.16 | -0.41+-0.16 | 1.66+-0.16 | Cr I |
Mn I | 3 | -3.79+-0.05 | -0.24+-0.05 | 1.60+-0.05 | -3.83+-0.05 | -0.26+-0.05 | 1.60+-0.05 | Mn I |
Fe I | 151 | -3.57+-0.15 | -0.02+-0.15 | 3.93+-0.15 | -3.57+-0.15 | -0.02+-0.15 | 3.93+-0.15 | Fe I |
Fe II | 10 | -3.54+-0.10 | 0.01+-0.10 | 3.96+-0.10 | -3.54+-0.10 | 0.01+-0.10 | 3.96+-0.10 | Fe II |
Co I | 4 | -3.00+-0.11 | 0.56+-0.11 | 1.92+-0.11 | -3.07+-0.11 | 0.50+-0.11 | 1.92+-0.11 | Co I |
Ni I | 3 | -3.34+-0.05 | 0.22+-0.05 | 2.91+-0.05 | -3.31+-0.05 | 0.26+-0.05 | 2.91+-0.05 | Ni I |
Zn I | 1 | -3.14 | 0.42 | 1.46 | -3.10 | 0.47 | 1.46 | Zn I |
Binary Parameters
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 | 14100 | 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 : 4850 | log g : 1.7 | 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 |
Li I | N/A | ... | ... | 0.52+-0.08 | -2.74+-0.08 | 0.82+-0.08 | 0.52+-0.08 | Li I |
C | N/A | -3.31+-0.06 | ... | ... | -3.22+-0.06 | 0.34+-0.06 | 5.21+-0.06 | C |
N | N/A | -3.32 | ... | ... | -3.23 | 0.33 | 4.60 | N |
[O I] | N/A | -2.66 | ... | ... | -2.61 | 0.95 | 6.08 | [O I] |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4840 | log g : 1.80+-0.34 | vturb : 1.90+-0.12 |
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 | ... | -3.18 | 0.06 | 5.25 | C |
Na | N/A | ... | -0.35 | ... | -3.67 | -0.43 | 2.57 | Na |
Mg | N/A | ... | -0.06 | ... | -3.49 | -0.25 | 4.11 | Mg |
Ca | N/A | ... | 0.10 | ... | -3.29 | -0.05 | 3.05 | Ca |
Fe I | N/A | -3.41 | ... | ... | -3.24 | ... | 4.26 | Fe I |
Fe II | N/A | -3.41 | ... | ... | -3.24 | ... | 4.26 | Fe II |
Ni | N/A | ... | 0.33 | ... | -3.05 | 0.19 | 3.17 | Ni |
Sr | N/A | ... | -1.80 | ... | -5.18 | -1.94 | -2.31 | Sr |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4850 | log g : 1.7 | 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 |
C | N/A | -3.30+-0.06 | ... | ... | -3.21+-0.06 | 0.35+-0.06 | 5.22+-0.06 | C |
N | N/A | -3.32+-0.10 | ... | ... | -3.23+-0.10 | 0.33+-0.10 | 4.60+-0.10 | N |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Isotopic Ratio
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4850 | log g : 1.7 | 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 |
Na | N/A | -3.90 | -0.34 | 2.35 | -3.89 | -0.33 | 2.35 | Na |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 |
A Search for Nitrogen-enhanced Metal-poor Stars
Stellar Parameters
Teff : 4892 | log g : 1.93 | vturb : 1.83 |
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+-0.29 | 5.36+-0.25 | -3.07+-0.25 | 0.21+-0.29 | 5.36+-0.25 | C |
N | N/A | ... | <0.13+-0.25 | <4.88+-0.25 | <-2.95+-0.25 | <0.33+-0.25 | <4.88+-0.25 | N |
Ca I | N/A | -3.35 | ... | ... | -3.33 | -0.05 | 3.01 | Ca I |
Ca II | N/A | -3.00 | ... | ... | -2.98 | 0.30 | 3.36 | Ca II |
Fe | N/A | -3.30+-0.21 | ... | ... | -3.28+-0.21 | ... | 4.22+-0.21 | Fe |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-09-04 | N/A | RCCTIO | N/A | 80 | 3600 | N/A |
NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4850 | log g : 1.7 | 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 |
Al | N/A | -3.72 | -0.16 | 2.75 | -3.70 | -0.14 | 2.75 | Al |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4850 | log g : 1.7 | 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 |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Ba | N/A | ... | ... | <-3.20 | <-5.38 | <-1.82 | <-3.20 | Ba |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4850 | log g : 1.7 | 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 |
Mg | N/A | ... | ... | 4.27 | -3.33 | 0.23 | 4.27 | Mg |
K | N/A | ... | ... | 1.83 | -3.20 | 0.36 | 1.83 | K |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4850 | log g : 1.7 | 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 |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Sr | 2 | ... | -1.80 | ... | -5.31 | -1.75 | -2.44 | Sr |
Y | N/A | ... | <-1.38 | ... | <-4.91 | <-1.35 | <-2.70 | Y |
Zr | N/A | ... | <-0.44 | ... | <-3.98 | <-0.42 | <-1.40 | Zr |
Ba | 1 | ... | -1.77 | ... | -5.38 | -1.82 | -3.20 | Ba |
La | 1 | ... | -0.11 | ... | -3.60 | -0.04 | -2.50 | La |
Ce | N/A | ... | <+0.48 | ... | <-3.08 | <0.48 | <-1.50 | Ce |
Pr | N/A | ... | <+0.40 | ... | <-3.17 | <0.39 | <-2.45 | Pr |
Nd | N/A | ... | <-0.14 | ... | <-3.62 | <-0.06 | <-2.20 | Nd |
Sm | N/A | ... | <+0.16 | ... | <-3.35 | <0.21 | <-2.39 | Sm |
Eu | N/A | ... | <+0.05 | ... | <-3.52 | <0.04 | <-3.00 | Eu |
Gd | N/A | ... | <+0.14 | ... | <-3.37 | <0.19 | <-2.30 | Gd |
Dy | N/A | ... | <-0.28 | ... | <-3.80 | <-0.24 | <-2.70 | Dy |
Ho | N/A | ... | <+0.10 | ... | <-3.67 | <-0.11 | <-3.20 | Ho |
Er | N/A | ... | <+0.43 | ... | <-3.12 | <0.44 | <-2.20 | Er |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4850 | log g : 1.7 | 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 |
Ca | N/A | -3.29 | 0.27 | ... | -3.27 | 0.29 | 3.07 | Ca |
Fe | N/A | -3.56 | ... | ... | -3.56 | ... | 3.94 | Fe |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | 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 : 4540+-34 | log g : 0.6+-0.14 | 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 | ... | ... | <0.37 | <-2.89 | <1.10 | <0.37 | Li I |
CH | 1 | ... | 0.25+-0.25 | 4.83 | -3.60 | 0.39+-0.25 | 4.83 | CH |
CN | 1 | ... | <1.47 | <5.45 | <-2.38 | <1.61 | <5.45 | CN |
O I | 3 | ... | <1.73 | <6.43 | <-2.26 | <1.73 | <6.43 | O I |
Na I | 2 | ... | -0.18+-0.17 | 2.07 | -4.17 | -0.18+-0.17 | 2.07 | Na I |
Mg I | 7 | ... | 0.57+-0.16 | 4.18 | -3.42 | 0.57+-0.16 | 4.18 | Mg I |
Al I | 1 | ... | -0.60+-0.26 | 1.86 | -4.59 | -0.60+-0.26 | 1.86 | Al I |
Ca I | 10 | ... | 0.25+-0.18 | 2.61 | -3.73 | 0.26+-0.18 | 2.61 | Ca I |
Sc II | 6 | ... | -0.11+-0.15 | -0.80 | -3.95 | 0.04+-0.15 | -0.80 | Sc II |
Ti I | 7 | ... | 0.00+-0.16 | 0.96 | -3.99 | 0.00+-0.16 | 0.96 | Ti I |
Ti II | 15 | ... | -0.16+-0.15 | 0.95 | -4.00 | -0.01+-0.15 | 0.95 | Ti II |
V I | 1 | ... | 0.05+-0.20 | -0.01 | -3.94 | 0.05+-0.20 | -0.01 | V I |
V II | 2 | ... | -0.09+-0.28 | -0.01 | -3.94 | 0.05+-0.28 | -0.01 | V II |
Cr I | 5 | ... | -0.39+-0.16 | 1.26 | -4.38 | -0.39+-0.16 | 1.26 | Cr I |
Cr II | 1 | ... | 0.25+-0.22 | 2.04 | -3.60 | 0.39+-0.22 | 2.04 | Cr II |
Mn I | 4 | ... | -0.16+-0.17 | 1.28 | -4.15 | -0.16+-0.17 | 1.28 | Mn I |
Fe I | 98 | -3.99+-0.15 | ... | 3.51 | -3.99+-0.15 | ... | 3.51 | Fe I |
Fe II | 7 | -3.85+-0.16 | ... | 3.65 | -3.85+-0.16 | ... | 3.65 | Fe II |
Co I | 5 | ... | 0.28+-0.20 | 1.28 | -3.71 | 0.28+-0.20 | 1.28 | Co I |
Ni I | 6 | ... | 0.37+-0.21 | 2.60 | -3.62 | 0.37+-0.21 | 2.60 | Ni I |
Zn I | 2 | ... | 0.70+-0.18 | 1.27 | -3.29 | 0.70+-0.18 | 1.27 | Zn I |
Rb I | 1 | ... | <3.02 | <1.55 | <-0.81 | <3.18 | <1.55 | Rb I |
Sr II | 2 | ... | -2.09+-0.15 | -3.06 | -5.93 | -1.94+-0.15 | -3.06 | Sr II |
Y II | 6 | ... | <-1.32 | <-2.96 | <-5.17 | <-1.18 | <-2.96 | Y II |
Zr II | 2 | ... | <-0.35 | <-1.62 | <-4.20 | <-0.21 | <-1.62 | Zr II |
Nb II | 1 | ... | <2.05 | <-0.34 | <-1.80 | <2.19 | <-0.34 | Nb II |
Mo I | 1 | ... | <1.35 | <-0.76 | <-2.64 | <1.35 | <-0.76 | Mo I |
Tc I | 1 | ... | ... | <-0.51 | <-0.51 | <3.48 | <-0.51 | Tc I |
Sn I | 1 | ... | <2.73 | <0.81 | <-1.26 | <2.73 | <0.81 | Sn I |
Ba II | 5 | ... | <-2.13 | <-3.80 | <-5.98 | <-1.99 | <-3.80 | Ba II |
La II | 3 | ... | <0.17 | <-2.58 | <-3.68 | <0.31 | <-2.58 | La II |
Ce II | 5 | ... | <0.06 | <-2.21 | <-3.79 | <0.20 | <-2.21 | Ce II |
Pr II | 4 | ... | <0.52 | <-2.61 | <-3.33 | <0.66 | <-2.61 | Pr II |
Nd II | 5 | ... | <0.07 | <-2.36 | <-3.78 | <0.21 | <-2.36 | Nd II |
Sm II | 2 | ... | <0.63 | <-2.26 | <-3.22 | <0.77 | <-2.26 | Sm II |
Eu II | 3 | ... | <-0.08 | <-3.41 | <-3.93 | <0.06 | <-3.41 | Eu II |
Gd II | 2 | ... | <0.96 | <-1.82 | <-2.89 | <1.10 | <-1.82 | Gd II |
Tb II | 3 | ... | <1.03 | <-2.52 | <-2.84 | <1.15 | <-2.52 | Tb II |
Dy II | 2 | ... | <0.41 | <-2.34 | <-3.44 | <0.55 | <-2.34 | Dy II |
Ho II | 1 | ... | <0.68 | <-2.69 | <-3.16 | <0.83 | <-2.69 | Ho II |
Er II | 2 | ... | <0.54 | <-2.39 | <-3.31 | <0.68 | <-2.39 | Er II |
Tm II | 2 | ... | <1.12 | <-2.63 | <-2.75 | <1.24 | <-2.63 | Tm II |
Yb II | 1 | ... | <0.02 | <-2.91 | <-3.83 | <0.16 | <-2.91 | Yb II |
Hf II | 1 | ... | <1.44 | <-1.56 | <-2.27 | <1.72 | <-1.56 | Hf II |
Pb I | 1 | ... | <2.22 | <0.27 | <-1.77 | <2.22 | <0.27 | Pb I |
Th II | 2 | ... | <1.18 | <-2.61 | <-2.67 | <1.32 | <-2.61 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | 159 |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-09-25-09:11 | 2453273.885 | MIKELCO | 41000 | 100-175 | 3600 | 159 |
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 | ... | -0.35 | ... | -3.67 | -0.26 | 2.57 | Na |
Mg | N/A | ... | -0.06 | ... | -3.49 | -0.08 | 4.11 | Mg |
Ca | N/A | ... | 0.1 | ... | -3.29 | 0.12 | 3.05 | Ca |
Ti | N/A | ... | 0.15 | ... | -3.19 | 0.22 | 1.76 | Ti |
Fe | N/A | -3.41 | ... | ... | -3.41 | ... | 4.09 | Fe |
Ni | N/A | ... | 0.33 | ... | -3.05 | 0.36 | 3.17 | Ni |
Position
Right Ascension : 03 06 29.51 | Declination : -54 30 32.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log