G17-25
taken from 6 paper(s):
/J.Simmerer et al.(2004)/
/D.Yong and D. L. Lambert(2003)/
/M.Ishigaki et al.(2010)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 4966 | log g : 4.26 | vturb : 0.80 |
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 | ... | -0.05 | ... | -1.41 | 0.13 | 7.02 | C |
Fe I | 16 | -1.54 | ... | ... | -1.54 | ... | 5.96 | Fe I |
Fe II | 9 | -1.44 | ... | ... | -1.44 | ... | 6.06 | Fe II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Magnesium Isotopic Abundance Ratios in Cool Stars
Stellar Parameters
Teff : 4950+-150 | log g : 4.50+-0.3 | vturb : 0.3+-0.3 |
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 | -1.46+-0.2 | ... | ... | -1.46+-0.2 | ... | 6.04+-0.2 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MCDONALD | 60000 | 90 | N/A | N/A |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5515+-69 | log g : 5.00 | vturb : 0.05 |
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 | N/A | -1.12+-0.05 | -0.22+-0.05 | ... | -1.03+-0.05 | -0.13+-0.05 | 5.21+-0.05 | Na I |
Mg I | N/A | -0.34+-0.05 | 0.57+-0.05 | ... | -0.36+-0.05 | 0.54+-0.05 | 7.24+-0.05 | Mg I |
Si | N/A | ... | 0.14+-0.05 | ... | -0.72+-0.05 | 0.18+-0.05 | 6.79+-0.05 | Si |
Si I | 2 | -0.77+-0.05 | ... | ... | -0.73+-0.05 | 0.17+-0.05 | 6.78+-0.05 | Si I |
Ca I | N/A | -0.64+-0.05 | 0.26+-0.05 | ... | -0.62+-0.05 | 0.28+-0.05 | 5.72+-0.05 | Ca I |
Ti | N/A | ... | 0.45+-0.04 | ... | -0.38+-0.04 | 0.52+-0.04 | 4.57+-0.04 | Ti |
Ti I | 2 | -0.49+-0.05 | ... | ... | -0.42+-0.05 | 0.48+-0.05 | 4.53+-0.05 | Ti I |
Ti II | 2 | -0.43+-0.05 | ... | ... | -0.36+-0.05 | 0.54+-0.05 | 4.59+-0.05 | Ti II |
Cr | N/A | ... | -0.02+-0.02 | ... | -0.89+-0.02 | 0.01+-0.02 | 4.75+-0.02 | Cr |
Cr I | 5 | -0.92+-0.02 | ... | ... | -0.89+-0.02 | 0.01+-0.02 | 4.75+-0.02 | Cr I |
Cr II | 1 | -0.97+-0.05 | ... | ... | -0.94+-0.05 | -0.04+-0.05 | 4.70+-0.05 | Cr II |
Mn I | N/A | -1.35+-0.07 | 0.07+-0.07 | ... | -1.39+-0.07 | -0.49+-0.07 | 4.04+-0.07 | Mn I |
Fe I | 17 | -0.90+-0.01 | ... | ... | -0.90+-0.01 | ... | 6.60+-0.01 | Fe I |
Fe II | 3 | -1.15+-0.10 | ... | ... | -1.15+-0.10 | ... | 6.35+-0.10 | Fe II |
Ni I | N/A | -0.85+-0.11 | 0.05+-0.11 | ... | -0.82+-0.11 | 0.08+-0.11 | 5.40+-0.11 | Ni I |
Zn I | N/A | -1.09+-0.06 | -0.18+-0.06 | ... | -1.05+-0.06 | -0.15+-0.06 | 3.51+-0.06 | Zn I |
Y II | N/A | -0.67+-0.05 | 0.24+-0.05 | ... | -0.64+-0.05 | 0.26+-0.05 | 1.57+-0.05 | Y II |
Ba II | N/A | -0.72+-0.05 | 0.19+-0.05 | ... | -0.77+-0.05 | 0.13+-0.05 | 1.41+-0.05 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | 304 | 1800 | -176.2+-0.4 |
THE UBIQUITY OF THE RAPID NEUTRON-CAPTURE PROCESS
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 | -1.54 | ... | ... | -1.54 | ... | 5.96 | Fe |
Zn I | N/A | ... | ... | 3.4 | -1.16 | 0.38 | 3.4 | Zn I |
Y II | N/A | ... | ... | 0.87 | -1.34 | 0.20 | 0.87 | Y II |
Pb I | N/A | ... | ... | 0.64 | -1.40 | 0.14 | 0.64 | Pb I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. I. Implications of [alpha/Fe] for Star Formation Histories in Their Progenitors
Stellar Parameters
Teff : 5174+-100 | log g : 4.85+-0.3 | vturb : 0.04+-0.3 |
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 | ... | 0.38+-0.12 | ... | -0.73+-0.12 | 0.38+-0.12 | 6.87+-0.12 | Mg |
Si | N/A | ... | 0.43+-0.16 | ... | -0.68+-0.16 | 0.43+-0.16 | 6.83+-0.16 | Si |
Ca | N/A | ... | 0.21+-0.08 | ... | -0.90+-0.08 | 0.21+-0.08 | 5.44+-0.08 | Ca |
Ti I | N/A | ... | 0.32+-0.11 | ... | -0.79+-0.11 | 0.32+-0.11 | 4.16+-0.11 | Ti I |
Ti II | N/A | ... | 0.43+-0.10 | ... | -0.68+-0.10 | 0.43+-0.10 | 4.27+-0.10 | Ti II |
Fe I | N/A | -1.11+-0.21 | ... | ... | -1.11+-0.21 | ... | 6.39+-0.21 | Fe I |
Fe II | N/A | -1.14+-0.12 | ... | ... | -1.14+-0.12 | ... | 6.36+-0.12 | Fe II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | -179.1+-0.3 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 5174 | log g : 4.85 | vturb : 0.04 |
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 | N/A | ... | -0.06+-0.1 | ... | -1.23+-0.1 | -0.06+-0.1 | 5.01+-0.1 | Na I |
Sc II | N/A | ... | 0.2+-0.12 | ... | -0.97+-0.12 | 0.20+-0.12 | 2.18+-0.12 | Sc II |
V I | N/A | ... | 0.09+-0.15 | ... | -1.08+-0.15 | 0.09+-0.15 | 2.85+-0.15 | V I |
Cr I | N/A | ... | -0.03+-0.13 | ... | -1.20+-0.13 | -0.03+-0.13 | 4.44+-0.13 | Cr I |
Cr II | N/A | ... | 0.23+-0.09 | ... | -0.94+-0.09 | 0.23+-0.09 | 4.70+-0.09 | Cr II |
Mn I | N/A | ... | -0.04+-0.23 | ... | -1.21+-0.23 | -0.04+-0.23 | 4.22+-0.23 | Mn I |
Fe I | N/A | -1.17+-0.17 | ... | ... | -1.17+-0.17 | ... | 6.33+-0.17 | Fe I |
Fe II | N/A | -1.08+-0.16 | ... | ... | -1.08+-0.16 | ... | 6.42+-0.16 | Fe II |
Ni I | N/A | ... | 0.04+-0.1 | ... | -1.13+-0.1 | 0.04+-0.1 | 5.09+-0.1 | Ni I |
Cu I | N/A | ... | -0.15+-0.12 | ... | -1.32+-0.12 | -0.15+-0.12 | 2.87+-0.12 | Cu I |
Zn I | N/A | ... | 0.28+-0.14 | ... | -0.89+-0.14 | 0.28+-0.14 | 3.67+-0.14 | Zn I |
Ba II | N/A | ... | 0.28+-0.23 | ... | -0.89+-0.23 | 0.28+-0.23 | 1.29+-0.23 | Ba II |
Nd II | N/A | ... | 0.89+-0.39 | ... | -0.28+-0.39 | 0.89+-0.39 | 1.14+-0.39 | Nd II |
Sm II | N/A | ... | 0.26+-0.15 | ... | -0.91+-0.15 | 0.26+-0.15 | 0.05+-0.15 | Sm II |
Eu II | N/A | ... | 0.23+-0.21 | ... | -0.94+-0.21 | 0.23+-0.21 | -0.42+-0.21 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | N/A | N/A |