BD+17_3248
HIP85487 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 19 paper(s):
/J.J.Cowan et al.(2002)/
/D.L.Burris et al.(2000)/
/R.Cayrel et al.(2004)/
/M.Spite et al.(2005)/
/J.A.Johnson(2002)/
/J.P.Fulbright and J. A. Johnson(2003)/
/J.J.Cowan et al.(2005)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/S.M.Andrievsky et al.(2008)/
/J.A.Johnson and M. Bolte(2002)/
/J.A.Johnson and M. Bolte(2001)/
/I.U.Roederer et al.(2009)/
/S.M.Andrievsky et al.(2009)/
/S.M.Andrievsky et al.(2010)/
/M.Spite et al.(2011)/
/P.Francois et al.(2007)/
/I.U.Roederer et al.(2012)/
/M.Spite et al.(2012)/
THE CHEMICAL COMPOSITION AND AGE OF THE METAL-POOR HALO STAR BD +173248
Stellar Parameters
Teff : 5200+-150 | log g : 1.80+-0.3 | vturb : 1.9+-0.2 |
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 | 1 | ... | ... | 0.2 | -3.06 | -1.00 | 0.2 | Li I |
CH | N/A | ... | -0.47+-0.15 | 6.00+-0.15 | -2.43+-0.15 | -0.37+-0.15 | 6.00+-0.15 | CH |
O I | 1 | ... | 0.46+-0.15 | 7.30+-0.15 | -1.39+-0.15 | 0.67+-0.15 | 7.30+-0.15 | O I |
Na I | 4 | ... | -0.05+-0.04 | 4.19+-0.04 | -2.05+-0.04 | 0.01+-0.04 | 4.19+-0.04 | Na I |
Mg I | 3 | ... | 0.41+-0.10 | 5.90+-0.10 | -1.70+-0.10 | 0.36+-0.10 | 5.90+-0.10 | Mg I |
Al I | 1 | ... | -0.69+-0.15 | 3.69+-0.15 | -2.76+-0.15 | -0.70+-0.15 | 3.69+-0.15 | Al I |
Si I | 6 | ... | 0.49+-0.11 | 5.95+-0.11 | -1.56+-0.11 | 0.50+-0.11 | 5.95+-0.11 | Si I |
Ca I | 19 | ... | 0.41+-0.06 | 4.68+-0.06 | -1.66+-0.06 | 0.40+-0.06 | 4.68+-0.06 | Ca I |
Sc II | 5 | ... | 0.16+-0.05 | 1.17+-0.05 | -1.98+-0.05 | 0.08+-0.05 | 1.17+-0.05 | Sc II |
Ti I | 13 | ... | 0.33+-0.09 | 3.23+-0.09 | -1.72+-0.09 | 0.34+-0.09 | 3.23+-0.09 | Ti I |
Ti II | 19 | ... | 0.37+-0.13 | 3.27+-0.13 | -1.68+-0.13 | 0.38+-0.13 | 3.27+-0.13 | Ti II |
V I | 2 | ... | -0.05+-0.01 | 1.86+-0.01 | -2.07+-0.01 | -0.01+-0.01 | 1.86+-0.01 | V I |
Cr I | 5 | ... | -0.13+-0.06 | 3.45+-0.06 | -2.19+-0.06 | -0.13+-0.06 | 3.45+-0.06 | Cr I |
Cr II | 4 | ... | 0.11+-0.09 | 3.69+-0.09 | -1.95+-0.09 | 0.11+-0.09 | 3.69+-0.09 | Cr II |
Mn I | 2 | ... | -0.28+-0.15 | 3.02+-0.15 | -2.41+-0.15 | -0.35+-0.15 | 3.02+-0.15 | Mn I |
Fe I | 139 | -2.08+-0.08 | ... | 5.44+-0.08 | -2.06+-0.08 | ... | 5.44+-0.08 | Fe I |
Fe II | 24 | -2.10+-0.09 | ... | 5.42+-0.09 | -2.08+-0.09 | ... | 5.42+-0.09 | Fe II |
Co I | 1 | ... | 0.09+-0.15 | 2.92+-0.15 | -2.07+-0.15 | -0.01+-0.15 | 2.92+-0.15 | Co I |
Ni I | 4 | ... | -0.06+-0.16 | 4.10+-0.16 | -2.12+-0.16 | -0.06+-0.16 | 4.10+-0.16 | Ni I |
Cu I | 1 | ... | -0.81+-0.15 | 1.31+-0.15 | -2.88+-0.15 | -0.82+-0.15 | 1.31+-0.15 | Cu I |
Zn I | 1 | ... | 0.07+-0.15 | 2.58+-0.15 | -1.98+-0.15 | 0.08+-0.15 | 2.58+-0.15 | Zn I |
Ge I | 1 | ... | -0.72+-0.15 | 0.60+-0.15 | -3.05+-0.15 | -0.99+-0.15 | 0.60+-0.15 | Ge I |
Sr I | 1 | ... | 0.09+-0.15 | 0.90+-0.15 | -1.97+-0.15 | 0.09+-0.15 | 0.90+-0.15 | Sr I |
Sr II | 2 | ... | 0.29+-0.10 | 1.10+-0.10 | -1.77+-0.10 | 0.29+-0.10 | 1.10+-0.10 | Sr II |
Y II | 11 | ... | -0.11+-0.05 | 0.04+-0.05 | -2.17+-0.05 | -0.11+-0.05 | 0.04+-0.05 | Y II |
Zr II | 19 | ... | 0.25+-0.14 | 0.76+-0.14 | -1.82+-0.14 | 0.24+-0.14 | 0.76+-0.14 | Zr II |
Nb II | 1 | ... | 0.49+-0.15 | -0.18+-0.15 | -1.64+-0.15 | 0.42+-0.15 | -0.18+-0.15 | Nb II |
Pd I | 3 | ... | 0.64+-0.09 | 0.24+-0.09 | -1.33+-0.09 | 0.73+-0.09 | 0.24+-0.09 | Pd I |
Ag I | 2 | ... | 0.57+-0.11 | -0.28+-0.11 | -1.48+-0.11 | 0.58+-0.11 | -0.28+-0.11 | Ag I |
Ba II | 6 | ... | 0.40+-0.11 | 0.44+-0.11 | -1.74+-0.11 | 0.32+-0.11 | 0.44+-0.11 | Ba II |
La II | 15 | ... | 0.45+-0.05 | -0.42+-0.05 | -1.52+-0.05 | 0.54+-0.05 | -0.42+-0.05 | La II |
Ce II | 22 | ... | 0.36+-0.06 | -0.18+-0.06 | -1.76+-0.06 | 0.30+-0.06 | -0.18+-0.06 | Ce II |
Pr II | 9 | ... | 0.67+-0.05 | -0.71+-0.05 | -1.43+-0.05 | 0.63+-0.05 | -0.71+-0.05 | Pr II |
Nd II | 40 | ... | 0.52+-0.17 | -0.07+-0.17 | -1.49+-0.17 | 0.57+-0.17 | -0.07+-0.17 | Nd II |
Sm II | 17 | ... | 0.67+-0.14 | -0.42+-0.14 | -1.38+-0.14 | 0.68+-0.14 | -0.42+-0.14 | Sm II |
Eu II | 9 | ... | 0.91+-0.05 | -0.67+-0.05 | -1.19+-0.05 | 0.87+-0.05 | -0.67+-0.05 | Eu II |
Gd II | 15 | ... | 0.71+-0.09 | -0.26+-0.09 | -1.33+-0.09 | 0.73+-0.09 | -0.26+-0.09 | Gd II |
Tb II | 5 | ... | 0.85+-0.05 | -0.91+-0.05 | -1.23+-0.05 | 0.83+-0.05 | -0.91+-0.05 | Tb II |
Dy II | 19 | ... | 0.96+-0.07 | -0.03+-0.07 | -1.13+-0.07 | 0.93+-0.07 | -0.03+-0.07 | Dy II |
Ho II | 3 | ... | 0.89+-0.17 | -0.70+-0.17 | -1.17+-0.17 | 0.89+-0.17 | -0.70+-0.17 | Ho II |
Er II | 7 | ... | 0.96+-0.06 | -0.20+-0.06 | -1.12+-0.06 | 0.94+-0.06 | -0.20+-0.06 | Er II |
Tm II | 2 | ... | 0.89+-0.10 | -1.07+-0.10 | -1.19+-0.10 | 0.87+-0.10 | -1.07+-0.10 | Tm II |
Os I | 2 | ... | 1.1+-0.10 | 0.45+-0.10 | -0.95+-0.10 | 1.11+-0.10 | 0.45+-0.10 | Os I |
Ir I | 3 | ... | 1.09+-0.13 | 0.30+-0.13 | -1.08+-0.13 | 0.98+-0.13 | 0.30+-0.13 | Ir I |
Pt I | 5 | ... | 0.96+-0.07 | 0.67+-0.07 | -0.95+-0.07 | 1.11+-0.07 | 0.67+-0.07 | Pt I |
Au I | 1 | ... | 0.8+-0.30 | -0.3+-0.30 | -1.10+-0.30 | 0.96+-0.30 | -0.3+-0.30 | Au I |
Pb I | 2 | ... | <0.5+-0.25 | <0.3+-0.25 | <-1.74+-0.25 | <0.32+-0.25 | <0.3+-0.25 | Pb I |
Th II | 2 | ... | 0.79+-0.10 | -1.18+-0.10 | -1.24+-0.10 | 0.82+-0.10 | -1.18+-0.10 | Th II |
U II | 1 | ... | 0.0+-0.30 | -2.0+-0.30 | -1.46+-0.30 | 0.60+-0.30 | -2.0+-0.30 | U II |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 | HST | 30000 | >50 | 10800 | N/A |
| N/A | KECKHIRES | 45000 | 30-300 | N/A | N/A |
| N/A | MCDONALD | 60000 | 130-250 | N/A | N/A |
NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS
Stellar Parameters
Teff : 5250 | log g : 2.30 | vturb : 1.50 |
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 | -2.02 | ... | ... | -1.85 | ... | 5.65 | Fe |
Sr | N/A | ... | 0.55 | 1.43 | -1.44 | 0.41 | 1.43 | Sr |
Y | N/A | ... | 0.06 | 0.28 | -1.93 | -0.08 | 0.28 | Y |
Zr | N/A | ... | 0.50 | 1.08 | -1.50 | 0.35 | 1.08 | Zr |
Ba | N/A | ... | 0.97 | 1.08 | -1.10 | 0.75 | 1.08 | Ba |
La | N/A | ... | 0.60 | -0.20 | -1.30 | 0.55 | -0.20 | La |
Nd | N/A | ... | 0.88 | 0.36 | -1.06 | 0.79 | 0.36 | Nd |
Eu | N/A | ... | 0.96 | -0.55 | -1.07 | 0.78 | -0.55 | Eu |
Dy | N/A | ... | 0.96 | 0.04 | -1.06 | 0.79 | 0.04 | Dy |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 | MAYALLKPNO | 20000 | 100-200 | N/A | N/A |
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Stellar Parameters
Teff : 5250 | log g : 1.4 | 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 | -2.50 | -0.44 | 6.02 | -2.41 | -0.37 | 6.02 | CH |
CN | N/A | -1.50 | 0.57 | 6.42 | -1.41 | 0.63 | 6.42 | CN |
[O I] | N/A | -1.38 | 0.69 | 7.39 | -1.30 | 0.74 | 7.39 | [O I] |
Na I | 2 | -1.38 | 0.69 | 4.95 | -1.29 | 0.75 | 4.95 | Na I |
Mg I | 7 | -1.88+-0.10 | 0.19+-0.10 | 5.70+-0.10 | -1.90+-0.10 | 0.14+-0.10 | 5.70+-0.10 | Mg I |
Al I | 2 | -2.77 | -0.71 | 3.70 | -2.75 | -0.71 | 3.70 | Al I |
Si I | 2 | -1.55 | 0.52 | 6.00 | -1.51 | 0.53 | 6.00 | Si I |
K I | 2 | -1.24 | 0.82 | 3.88 | -1.15 | 0.89 | 3.88 | K I |
Ca I | 14 | -1.67+-0.08 | 0.40+-0.08 | 4.69+-0.08 | -1.65+-0.08 | 0.39+-0.08 | 4.69+-0.08 | Ca I |
Sc II | 6 | -1.87+-0.16 | 0.20+-0.16 | 1.30+-0.16 | -1.85+-0.16 | 0.19+-0.16 | 1.30+-0.16 | Sc II |
Ti I | 12 | -1.84+-0.08 | 0.23+-0.08 | 3.18+-0.08 | -1.77+-0.08 | 0.27+-0.08 | 3.18+-0.08 | Ti I |
Ti II | 29 | -1.74+-0.17 | 0.33+-0.17 | 3.28+-0.17 | -1.67+-0.17 | 0.37+-0.17 | 3.28+-0.17 | Ti II |
Cr I | 6 | -2.28+-0.20 | -0.22+-0.20 | 3.39+-0.20 | -2.25+-0.20 | -0.21+-0.20 | 3.39+-0.20 | Cr I |
Mn I | 3 | -2.53+-0.02 | -0.47+-0.02 | 2.86+-0.02 | -2.57+-0.02 | -0.53+-0.02 | 2.86+-0.02 | Mn I |
Fe I | 141 | -2.04+-0.15 | 0.02+-0.15 | 5.46+-0.15 | -2.04+-0.15 | 0.02+-0.15 | 5.46+-0.15 | Fe I |
Fe II | 16 | -2.09+-0.09 | -0.03+-0.09 | 5.41+-0.09 | -2.09+-0.09 | -0.03+-0.09 | 5.41+-0.09 | Fe II |
Co I | 2 | -1.71 | 0.36 | 3.21 | -1.78 | 0.26 | 3.21 | Co I |
Ni I | 3 | -2.06+-0.08 | 0.00+-0.08 | 4.19+-0.08 | -2.03+-0.08 | 0.01+-0.08 | 4.19+-0.08 | Ni I |
Zn I | 1 | -2.06 | 0.00 | 2.54 | -2.02 | 0.02 | 2.54 | Zn I |
Binary Parameters
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 | 160 | 2700 | N/A |
2001-06 | N/A | VLT | N/A | N/A | N/A | N/A |
2001-09 | N/A | VLT | N/A | 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 : 5250 | log g : 1.4 | 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 |
Li I | N/A | ... | ... | <0.00 | <-3.26 | <-1.19 | <0.00 | Li I |
C | N/A | -2.44+-0.05 | ... | ... | -2.35+-0.05 | -0.28+-0.05 | 6.08+-0.05 | C |
N | N/A | -1.42 | ... | ... | -1.33 | 0.74 | 6.50 | N |
[O I] | N/A | -1.38 | ... | ... | -1.33 | 0.74 | 7.36 | [O I] |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 |
ABUNDANCES OF 30 ELEMENTS IN 23 METAL-POOR STARS
Stellar Parameters
Teff : 5200 | log g : 1.80 | vturb : 1.90 |
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 | ... | ... | 4.76+-0.21 | -1.48+-0.21 | 0.61+-0.21 | 4.76+-0.21 | Na I |
Mg I | 5 | ... | ... | 6.10+-0.11 | -1.50+-0.11 | 0.59+-0.11 | 6.10+-0.11 | Mg I |
Al I | 1 | ... | ... | 3.71+-0.25 | -2.74+-0.25 | -0.65+-0.25 | 3.71+-0.25 | Al I |
Si I | 1 | ... | ... | 5.72+-0.23 | -1.79+-0.23 | 0.30+-0.23 | 5.72+-0.23 | Si I |
Ca I | 21 | ... | ... | 4.65+-0.08 | -1.69+-0.08 | 0.40+-0.08 | 4.65+-0.08 | Ca I |
Sc II | 10 | ... | ... | 1.17+-0.16 | -1.98+-0.16 | 0.11+-0.16 | 1.17+-0.16 | Sc II |
Ti I | 19 | ... | ... | 3.13+-0.11 | -1.82+-0.11 | 0.27+-0.11 | 3.13+-0.11 | Ti I |
Ti II | 16 | ... | ... | 3.20+-0.16 | -1.75+-0.16 | 0.34+-0.16 | 3.20+-0.16 | Ti II |
V I | 3 | ... | ... | 1.79+-0.12 | -2.14+-0.12 | -0.05+-0.12 | 1.79+-0.12 | V I |
V II | 1 | ... | ... | 2.10+-0.17 | -1.83+-0.17 | 0.26+-0.17 | 2.10+-0.17 | V II |
Cr I | 12 | ... | ... | 3.49+-0.11 | -2.15+-0.11 | -0.06+-0.11 | 3.49+-0.11 | Cr I |
Cr II | 2 | ... | ... | 3.79+-0.11 | -1.85+-0.11 | 0.24+-0.11 | 3.79+-0.11 | Cr II |
Mn I | 4 | ... | ... | 3.01+-0.10 | -2.42+-0.10 | -0.33+-0.10 | 3.01+-0.10 | Mn I |
Fe I | 139 | ... | ... | 5.41+-0.13 | -2.09+-0.13 | ... | 5.41+-0.13 | Fe I |
Fe II | 22 | ... | ... | 5.41+-0.14 | -2.09+-0.14 | ... | 5.41+-0.14 | Fe II |
Co I | 4 | ... | ... | 2.96+-0.21 | -2.03+-0.21 | 0.06+-0.21 | 2.96+-0.21 | Co I |
Ni I | 8 | ... | ... | 4.19+-0.13 | -2.03+-0.13 | 0.06+-0.13 | 4.19+-0.13 | Ni I |
Zn I | 1 | ... | ... | 2.55+-0.09 | -2.01+-0.09 | 0.08+-0.09 | 2.55+-0.09 | Zn I |
Y II | 5 | ... | ... | 0.10+-0.16 | -2.11+-0.16 | -0.02+-0.16 | 0.10+-0.16 | Y II |
Zr II | 1 | ... | ... | 0.75+-0.18 | -1.83+-0.18 | 0.26+-0.18 | 0.75+-0.18 | Zr II |
Ba II | 4 | ... | ... | 0.51+-0.26 | -1.67+-0.26 | 0.42+-0.26 | 0.51+-0.26 | Ba II |
La II | 3 | ... | ... | -0.53+-0.14 | -1.63+-0.14 | 0.46+-0.14 | -0.53+-0.14 | La II |
Ce II | 2 | ... | ... | -0.21+-0.14 | -1.79+-0.14 | 0.30+-0.14 | -0.21+-0.14 | Ce II |
Nd II | 8 | ... | ... | -0.06+-0.16 | -1.48+-0.16 | 0.61+-0.16 | -0.06+-0.16 | Nd II |
Sm II | 4 | ... | ... | -0.26+-0.16 | -1.22+-0.16 | 0.87+-0.16 | -0.26+-0.16 | Sm II |
Eu II | 1 | ... | ... | -0.80+-0.24 | -1.32+-0.24 | 0.77+-0.24 | -0.80+-0.24 | Eu II |
Tb II | N/A | ... | ... | <1.32 | <1.00 | <3.09 | <1.32 | Tb II |
Dy II | 2 | ... | ... | -0.13+-0.20 | -1.23+-0.20 | 0.86+-0.20 | -0.13+-0.20 | Dy II |
Os I | N/A | ... | ... | <0.84 | <-0.56 | <1.53 | <0.84 | Os I |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-08-12 | N/A | LICKHAMILTON | 60000 | 80 | 1800 | N/A |
Oxygen Abundances in Metal-poor Stars
Stellar Parameters
Teff : 5025 | log g : 2.23 | 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 |
O I | N/A | ... | 0.55+-0.1 | 7.21+-0.13 | -1.48+-0.13 | 0.53+-0.1 | 7.21+-0.13 | O I |
Fe | N/A | -2.03 | ... | ... | -2.01 | ... | 5.49 | Fe |
Fe I | N/A | ... | ... | 5.27+-0.06 | -2.23+-0.06 | ... | 5.27+-0.06 | Fe I |
Fe II | N/A | ... | ... | 5.49+-0.03 | -2.01+-0.03 | ... | 5.49+-0.03 | Fe II |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-05 | N/A | GECKOCFHT | 130000 | 300 | 1800 | N/A |
2001-09-30 | N/A | GECKOCFHT | 130000 | N/A | 1800 | N/A |
Hubble Space Telescope Observations of Heavy Elements in Metal-Poor Galactic Halo Stars
Stellar Parameters
Teff : 5200 | log g : 1.80 | vturb : 1.90 |
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 | N/A | -2.08 | ... | ... | -2.11 | ... | 5.39 | Fe I |
Fe II | N/A | -2.10 | ... | ... | -2.13 | ... | 5.37 | Fe II |
Ge | N/A | ... | -1.06 | +0.46 | -3.19 | -1.08 | +0.46 | Ge |
Zr | N/A | ... | +0.14 | +0.64 | -1.94 | 0.17 | +0.64 | Zr |
La | N/A | ... | +0.52 | -0.42 | -1.52 | 0.59 | -0.42 | La |
Eu | N/A | ... | +0.91 | -0.67 | -1.19 | 0.92 | -0.67 | Eu |
Os | N/A | ... | +1.04 | +0.37 | -1.03 | 1.08 | +0.37 | Os |
Ir | N/A | ... | +0.95 | +0.23 | -1.15 | 0.96 | +0.23 | Ir |
Pt | N/A | ... | +0.88 | +0.50 | -1.12 | 0.99 | +0.50 | Pt |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 | HST | 30000 | >50 | N/A | N/A |
| N/A | KECKHIRES | 45000 | 30-200 | 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 : 5250 | log g : 1.4 | 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 |
C | N/A | -2.40+-0.05 | ... | ... | -2.31+-0.05 | -0.24+-0.05 | 6.12+-0.05 | C |
N | N/A | -1.42+-0.10 | ... | ... | -1.33+-0.10 | 0.74+-0.10 | 6.50+-0.10 | N |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Isotopic Ratio
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 : 5250 | log g : 1.4 | 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 |
Na | N/A | -1.81 | +0.26 | 4.44 | -1.80 | 0.27 | 4.44 | Na |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 : 5250 | log g : 1.4 | 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 |
Al | N/A | -1.97 | 0.1 | 4.5 | -1.95 | 0.12 | 4.5 | Al |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 r-Process in the Early Galaxy
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 | -2.10 | ... | ... | -1.93 | ... | 5.57 | Fe |
Sr II | N/A | ... | ... | 0.94+-0.30 | -1.93+-0.30 | -0.00+-0.30 | 0.94+-0.30 | Sr II |
Y II | N/A | ... | ... | 0.10+-0.16 | -2.11+-0.16 | -0.18+-0.16 | 0.10+-0.16 | Y II |
Zr II | N/A | ... | ... | 0.75+-0.18 | -1.83+-0.18 | 0.10+-0.18 | 0.75+-0.18 | Zr II |
Ba II | N/A | ... | ... | 0.51+-0.14 | -1.67+-0.14 | 0.26+-0.14 | 0.51+-0.14 | Ba II |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-08-12 | N/A | LICKHAMILTON | 60000 | 80 | 1800 | N/A |
Th Ages for Metal-poor Stars
Stellar Parameters
Teff : 5200 | log g : 1.80 | vturb : 1.90 |
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 | 139 | -2.11+-0.13 | ... | ... | -1.94+-0.13 | ... | 5.56+-0.13 | Fe I |
Fe II | 22 | -2.11+-0.14 | ... | ... | -1.94+-0.14 | ... | 5.56+-0.14 | Fe II |
Ba II | 4 | ... | 0.49+-0.26 | ... | -1.67+-0.26 | 0.27+-0.26 | 0.51+-0.26 | Ba II |
La II | 3 | ... | 0.36+-0.14 | ... | -1.63+-0.14 | 0.31+-0.14 | -0.53+-0.14 | La II |
Ce II | 2 | ... | 0.35+-0.14 | ... | -1.73+-0.14 | 0.21+-0.14 | -0.15+-0.14 | Ce II |
Nd II | 8 | ... | 0.55+-0.16 | ... | -1.48+-0.16 | 0.46+-0.16 | -0.06+-0.16 | Nd II |
Sm II | 4 | ... | 0.85+-0.16 | ... | -1.22+-0.16 | 0.72+-0.16 | -0.26+-0.16 | Sm II |
Eu II | 1 | ... | 0.80+-0.24 | ... | -1.32+-0.24 | 0.62+-0.24 | -0.80+-0.24 | Eu II |
Tb II | N/A | ... | <1.32 | ... | <-0.78 | <1.16 | <-0.46 | Tb II |
Dy II | 2 | ... | 0.88+-0.20 | ... | -1.23+-0.20 | 0.71+-0.20 | -0.13+-0.20 | Dy II |
Os I | N/A | ... | <1.50 | ... | <-0.56 | <1.38 | <0.84 | Os I |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-08-12 | N/A | LICKHAMILTON | 60000 | 80 | 1800 | N/A |
The End of Nucleosynthesis: Production of Lead and Thorium in the Early Galaxy
Stellar Parameters
Teff : 5200 | log g : 1.80 | vturb : 1.90 |
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 | -2.08 | ... | ... | -2.08 | ... | 5.42 | Fe |
La II | N/A | ... | ... | -0.55+-0.05 | -1.65+-0.05 | 0.43+-0.05 | -0.55+-0.05 | La II |
Eu II | N/A | ... | ... | -0.78+-0.05 | -1.30+-0.05 | 0.78+-0.05 | -0.78+-0.05 | Eu II |
Er II | N/A | ... | ... | -0.34+-0.07 | -1.26+-0.07 | 0.82+-0.07 | -0.34+-0.07 | Er II |
Hf II | N/A | ... | ... | -0.73+-0.11 | -1.44+-0.11 | 0.64+-0.11 | -0.73+-0.11 | Hf II |
Ir I | N/A | ... | ... | +0.12+-0.16 | -1.26+-0.16 | 0.82+-0.16 | +0.12+-0.16 | Ir I |
Pb I | N/A | ... | ... | <+0.27 | <-1.77 | <0.31 | <+0.27 | Pb I |
Th II | N/A | ... | ... | -1.26+-0.10 | -1.32+-0.10 | 0.76+-0.10 | -1.26+-0.10 | Th II |
Isotopic Ratio
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 | HST | 30000 | 50 | N/A | N/A |
| N/A | KECKHIRES | 45000 | 30-200 | 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 : 5250 | log g : 1.4 | 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 |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Ba | 3 | ... | ... | +0.75 | -1.43 | 0.64 | +0.75 | Ba |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 : 5250 | log g : 1.4 | 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 |
Mg | N/A | ... | ... | 6.00 | -1.60 | 0.47 | 6.00 | Mg |
K | N/A | ... | ... | 3.77 | -1.26 | 0.81 | 3.77 | K |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 : 5250 | log g : 1.4 | 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 |
S I | 2 | ... | ... | 5.57+-0.10 | -1.55+-0.10 | 0.52+-0.10 | 5.57+-0.10 | S I |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 : 5250 | log g : 1.4 | 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 |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Sr | 3 | ... | +0.05 | ... | -1.97 | 0.10 | 0.90 | Sr |
Y | 3 | ... | -0.02 | ... | -2.06 | 0.01 | 0.15 | Y |
Zr | 5 | ... | +0.53 | ... | -1.52 | 0.55 | 1.06 | Zr |
Ba | 2 | ... | +0.69 | ... | -1.43 | 0.64 | 0.75 | Ba |
La | 5 | ... | +0.66 | ... | -1.34 | 0.73 | -0.24 | La |
Ce | 2 | ... | +0.49 | ... | -1.58 | 0.49 | 0.00 | Ce |
Pr | 1 | ... | +0.66 | ... | -1.42 | 0.65 | -0.70 | Pr |
Nd | 2 | ... | +0.69 | ... | -1.30 | 0.77 | 0.12 | Nd |
Sm | 2 | ... | +0.74 | ... | -1.28 | 0.79 | -0.32 | Sm |
Eu | 3 | ... | +0.93 | ... | -1.15 | 0.92 | -0.63 | Eu |
Gd | 1 | ... | +0.90 | ... | -1.12 | 0.95 | -0.05 | Gd |
Dy | 2 | ... | +1.01 | ... | -1.02 | 1.05 | 0.08 | Dy |
Ho | 1 | ... | +0.91 | ... | -1.37 | 0.70 | -0.90 | Ho |
Er | 2 | ... | +1.24 | ... | -0.82 | 1.25 | 0.10 | Er |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 |
Detection of the Second r-process Peak Element Tellurium in Metal-poor Stars
Stellar Parameters
Teff : 5200 | log g : 1.80 | vturb : 1.90 |
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 | N/A | -2.08 | ... | ... | -2.08 | ... | 5.42 | Fe I |
Te | N/A | ... | +0.60+-0.30 | +0.70+-0.30 | -1.48+-0.30 | 0.60+-0.30 | +0.70+-0.30 | Te |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 | HST | 30000 | 100 | N/A | N/A |
NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
Stellar Parameters
Teff : 5250 | log g : 1.4 | 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 |
Ca | N/A | -1.62 | 0.45 | ... | -1.60 | 0.47 | 4.74 | Ca |
Fe | N/A | -2.07 | ... | ... | -2.07 | ... | 5.43 | Fe |
Position
Right Ascension : 17 28 14.47 | Declination : +17 30 35.9 | 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 |