G125-13
taken from 5 paper(s):
/M.Ishigaki et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5688+-82 | log g : 4.02 | vturb : 1.12 |
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 |
Na I | N/A | -1.85+-0.08 | -0.16+-0.08 | ... | -1.76+-0.08 | -0.07+-0.08 | 4.48+-0.08 | Na I |
Mg I | N/A | -1.30+-0.03 | 0.39+-0.04 | ... | -1.32+-0.03 | 0.37+-0.04 | 6.28+-0.03 | Mg I |
Ca I | N/A | -1.43+-0.03 | 0.26+-0.04 | ... | -1.41+-0.03 | 0.28+-0.04 | 4.93+-0.03 | Ca I |
Ti | N/A | ... | 0.31+-0.02 | ... | -1.31+-0.02 | 0.38+-0.02 | 3.64+-0.02 | Ti |
Ti I | 3 | -1.51+-0.02 | ... | ... | -1.44+-0.02 | 0.25+-0.02 | 3.51+-0.02 | Ti I |
Ti II | 6 | -1.23+-0.03 | ... | ... | -1.16+-0.03 | 0.53+-0.03 | 3.79+-0.03 | Ti II |
Cr | N/A | ... | -0.16+-0.02 | ... | -1.82+-0.02 | -0.13+-0.02 | 3.82+-0.02 | Cr |
Cr I | 5 | -1.89+-0.02 | ... | ... | -1.86+-0.02 | -0.17+-0.02 | 3.78+-0.02 | Cr I |
Cr II | 1 | -1.43+-0.07 | ... | ... | -1.40+-0.07 | 0.29+-0.07 | 4.24+-0.07 | Cr II |
Mn I | N/A | -2.23+-0.07 | 0.08+-0.08 | ... | -2.27+-0.07 | -0.58+-0.08 | 3.16+-0.07 | Mn I |
Fe I | 33 | -1.69+-0.02 | ... | ... | -1.69+-0.02 | ... | 5.81+-0.02 | Fe I |
Fe II | 7 | -1.69+-0.02 | ... | ... | -1.69+-0.02 | ... | 5.81+-0.02 | Fe II |
Ni I | N/A | -1.74+-0.03 | -0.05+-0.03 | ... | -1.71+-0.03 | -0.02+-0.03 | 4.51+-0.03 | Ni I |
Zn I | N/A | -1.77+-0.09 | -0.08+-0.09 | ... | -1.73+-0.09 | -0.04+-0.09 | 2.83+-0.09 | Zn I |
Y II | N/A | -1.82+-0.08 | -0.13+-0.08 | ... | -1.79+-0.08 | -0.10+-0.08 | 0.42+-0.08 | Y II |
Ba II | N/A | -1.88+-0.08 | -0.19+-0.08 | ... | -1.93+-0.08 | -0.24+-0.08 | 0.25+-0.08 | Ba II |
Position
Right Ascension : 19 31 09.23 | Declination : +36 09 10.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | 351 | 1200 | -175.0+-0.2 |
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 : 6079+-100 | log g : 4.75+-0.3 | vturb : 0.79+-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 | ... | 0.17+-0.09 | ... | -1.19+-0.09 | 0.17+-0.09 | 6.41+-0.09 | Mg |
Si | N/A | ... | 0.13+-0.11 | ... | -1.23+-0.11 | 0.13+-0.11 | 6.28+-0.11 | Si |
Ca | N/A | ... | 0.21+-0.07 | ... | -1.15+-0.07 | 0.21+-0.07 | 5.19+-0.07 | Ca |
Ti I | N/A | ... | 0.30+-0.07 | ... | -1.06+-0.07 | 0.30+-0.07 | 3.89+-0.07 | Ti I |
Ti II | N/A | ... | 0.39+-0.07 | ... | -0.97+-0.07 | 0.39+-0.07 | 3.98+-0.07 | Ti II |
Fe I | N/A | -1.36+-0.10 | ... | ... | -1.36+-0.10 | ... | 6.14+-0.10 | Fe I |
Fe II | N/A | -1.35+-0.11 | ... | ... | -1.35+-0.11 | ... | 6.15+-0.11 | Fe II |
Binary Parameters
Position
Right Ascension : 19 31 09.23 | Declination : +36 09 10.2 | 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 | SUBARUHDS | 50000 | N/A | N/A | -178.5+-0.5 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6079 | log g : 4.75 | vturb : 0.79 |
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 | ... | -0.2+-0.12 | ... | -1.55+-0.12 | -0.20+-0.12 | 4.69+-0.12 | Na I |
Sc II | N/A | ... | 0.1+-0.07 | ... | -1.25+-0.07 | 0.10+-0.07 | 1.90+-0.07 | Sc II |
V I | N/A | ... | 0.09+-0.14 | ... | -1.26+-0.14 | 0.09+-0.14 | 2.67+-0.14 | V I |
Cr I | N/A | ... | -0.14+-0.06 | ... | -1.49+-0.06 | -0.14+-0.06 | 4.15+-0.06 | Cr I |
Cr II | N/A | ... | 0.15+-0.08 | ... | -1.20+-0.08 | 0.15+-0.08 | 4.44+-0.08 | Cr II |
Mn I | N/A | ... | -0.32+-0.07 | ... | -1.67+-0.07 | -0.32+-0.07 | 3.76+-0.07 | Mn I |
Fe I | N/A | -1.35+-0.1 | ... | ... | -1.35+-0.1 | ... | 6.15+-0.1 | Fe I |
Fe II | N/A | -1.35+-0.11 | ... | ... | -1.35+-0.11 | ... | 6.15+-0.11 | Fe II |
Co I | N/A | ... | 0.17+-0.14 | ... | -1.18+-0.14 | 0.17+-0.14 | 3.81+-0.14 | Co I |
Ni I | N/A | ... | -0.07+-0.09 | ... | -1.42+-0.09 | -0.07+-0.09 | 4.80+-0.09 | Ni I |
Cu I | N/A | ... | -0.8 | ... | -2.15 | -0.80 | 2.04 | Cu I |
Zn I | N/A | ... | 0.03+-0.11 | ... | -1.32+-0.11 | 0.03+-0.11 | 3.24+-0.11 | Zn I |
Sr II | N/A | ... | -0.09+-0.21 | ... | -1.44+-0.21 | -0.09+-0.21 | 1.43+-0.21 | Sr II |
Y II | N/A | ... | -0.1+-0.09 | ... | -1.45+-0.09 | -0.10+-0.09 | 0.76+-0.09 | Y II |
Ba II | N/A | ... | -0.01+-0.15 | ... | -1.36+-0.15 | -0.01+-0.15 | 0.82+-0.15 | Ba II |
Nd II | N/A | ... | 0.38+-0.18 | ... | -0.97+-0.18 | 0.38+-0.18 | 0.45+-0.18 | Nd II |
Sm II | N/A | ... | 0.61+-0.12 | ... | -0.74+-0.12 | 0.61+-0.12 | 0.22+-0.12 | Sm II |
Eu II | N/A | ... | 0.52+-0.21 | ... | -0.83+-0.21 | 0.52+-0.21 | -0.31+-0.21 | Eu II |
Position
Right Ascension : 19 31 09.23 | Declination : +36 09 10.2 | 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 | SUBARUHDS | 50000 | N/A | N/A | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5848 | log g : 4.28 | 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 | ... | -0.17 | ... | -1.51 | -0.08 | 4.73 | Na |
Mg | N/A | ... | 0.3 | ... | -1.15 | 0.28 | 6.45 | Mg |
Si | N/A | ... | 0.28 | ... | -1.11 | 0.32 | 6.40 | Si |
Ca | N/A | ... | 0.3 | ... | -1.11 | 0.32 | 5.23 | Ca |
Ti | N/A | ... | 0.2 | ... | -1.16 | 0.27 | 3.79 | Ti |
Cr | N/A | ... | -0.09 | ... | -1.49 | -0.06 | 4.15 | Cr |
Fe | N/A | -1.43 | ... | ... | -1.43 | ... | 6.07 | Fe |
Ni | N/A | ... | -0.09 | ... | -1.49 | -0.06 | 4.73 | Ni |
Position
Right Ascension : 19 31 09.23 | Declination : +36 09 10.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-19-0249 | N/A | FIESNOT | 40000 | 175 | N/A | -175.9 |
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
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 |
Mn | N/A | ... | -0.38 | ... | -1.85 | -0.42 | 3.58 | Mn |
Fe | N/A | -1.43 | ... | ... | -1.43 | ... | 6.07 | Fe |
Zn | N/A | ... | 0.05 | ... | -1.34 | 0.09 | 3.22 | Zn |
Y | N/A | ... | -0.22 | ... | -1.62 | -0.19 | 0.59 | Y |
Ba | N/A | ... | -0.31 | ... | -1.79 | -0.36 | 0.39 | Ba |
Position
Right Ascension : 19 31 09.23 | Declination : +36 09 10.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-19-0249 | N/A | FIESNOT | 40000 | 175 | N/A | -175.9 |