G188-22
taken from 10 paper(s):
/J.R.Shi et al.(2007)/
/J.Simmerer et al.(2004)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/I.U.Roederer et al.(2014)/
/H.L.Yan et al.(2016)/
/A.M.Boesgaard et al.(2011)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Lithium abundances in metal-poor stars (Research Note)
Stellar Parameters
Teff : 6040 | log g : 4.37 | 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 |
Li I | N/A | ... | ... | 2.26 | -1.00 | 0.24 | 2.26 | Li I |
Fe | N/A | -1.25 | ... | ... | -1.24 | ... | 6.26 | Fe |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | 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 | FOCES | 40000 | 100-400 | N/A | N/A |
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 5827 | log g : 4.27 | vturb : 1.20 |
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 | ... | -0.35 | ... | -1.69 | -0.17 | 6.74 | C |
Fe I | 7 | -1.52 | ... | ... | -1.52 | ... | 5.98 | Fe I |
Fe II | 8 | -1.35 | ... | ... | -1.35 | ... | 6.15 | Fe II |
La II | N/A | ... | ... | -0.12+-0.05 | -1.22+-0.05 | 0.30+-0.05 | -0.12+-0.05 | La II |
Eu II | N/A | ... | ... | -0.6+-0.1 | -1.12+-0.1 | 0.40+-0.1 | -0.6+-0.1 | Eu II |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | 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 | MCDONALD | 60000 | 100 | N/A | N/A |
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 | -1.52 | ... | ... | -1.52 | ... | 5.98 | Fe |
Zn I | N/A | ... | ... | 3.24 | -1.32 | 0.20 | 3.24 | Zn I |
Y II | N/A | ... | ... | 0.94 | -1.27 | 0.25 | 0.94 | Y II |
Pb I | N/A | ... | ... | <+1.30 | <-0.74 | <0.78 | <+1.30 | Pb I |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | 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 | 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 : 6170+-100 | log g : 4.52+-0.3 | vturb : 1.13+-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 | ... | 0.28+-0.08 | ... | -0.99+-0.08 | 0.28+-0.08 | 6.61+-0.08 | Mg |
Si | N/A | ... | 0.29+-0.11 | ... | -0.98+-0.11 | 0.29+-0.11 | 6.53+-0.11 | Si |
Ca | N/A | ... | 0.26+-0.07 | ... | -1.01+-0.07 | 0.26+-0.07 | 5.33+-0.07 | Ca |
Ti I | N/A | ... | 0.35+-0.07 | ... | -0.92+-0.07 | 0.35+-0.07 | 4.03+-0.07 | Ti I |
Ti II | N/A | ... | 0.45+-0.08 | ... | -0.82+-0.08 | 0.45+-0.08 | 4.13+-0.08 | Ti II |
Fe I | N/A | -1.27+-0.10 | ... | ... | -1.27+-0.10 | ... | 6.23+-0.10 | Fe I |
Fe II | N/A | -1.28+-0.12 | ... | ... | -1.28+-0.12 | ... | 6.22+-0.12 | Fe II |
Binary Parameters
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | 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 | SUBARUHDS | 50000 | N/A | N/A | -95.7+-0.3 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6170 | log g : 4.52 | vturb : 1.13 |
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 | ... | 0.02+-0.11 | ... | -1.24+-0.11 | 0.02+-0.11 | 5.00+-0.11 | Na I |
Sc II | N/A | ... | 0.23+-0.07 | ... | -1.03+-0.07 | 0.23+-0.07 | 2.12+-0.07 | Sc II |
V I | N/A | ... | 0.1+-0.13 | ... | -1.16+-0.13 | 0.10+-0.13 | 2.77+-0.13 | V I |
Cr I | N/A | ... | -0.09+-0.07 | ... | -1.35+-0.07 | -0.09+-0.07 | 4.29+-0.07 | Cr I |
Cr II | N/A | ... | 0.19+-0.07 | ... | -1.07+-0.07 | 0.19+-0.07 | 4.57+-0.07 | Cr II |
Mn I | N/A | ... | -0.27+-0.12 | ... | -1.53+-0.12 | -0.27+-0.12 | 3.90+-0.12 | Mn I |
Fe I | N/A | -1.26+-0.1 | ... | ... | -1.26+-0.1 | ... | 6.24+-0.1 | Fe I |
Fe II | N/A | -1.29+-0.12 | ... | ... | -1.29+-0.12 | ... | 6.21+-0.12 | Fe II |
Ni I | N/A | ... | -0.02+-0.08 | ... | -1.28+-0.08 | -0.02+-0.08 | 4.94+-0.08 | Ni I |
Zn I | N/A | ... | 0.11+-0.1 | ... | -1.15+-0.1 | 0.11+-0.1 | 3.41+-0.1 | Zn I |
Y II | N/A | ... | 0.26+-0.08 | ... | -1.00+-0.08 | 0.26+-0.08 | 1.21+-0.08 | Y II |
Ba II | N/A | ... | 0.32+-0.15 | ... | -0.94+-0.15 | 0.32+-0.15 | 1.24+-0.15 | Ba II |
Nd II | N/A | ... | 0.55+-0.08 | ... | -0.71+-0.08 | 0.55+-0.08 | 0.71+-0.08 | Nd II |
Eu II | N/A | ... | 0.33+-0.21 | ... | -0.93+-0.21 | 0.33+-0.21 | -0.41+-0.21 | Eu II |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | 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 | SUBARUHDS | 50000 | N/A | N/A | N/A |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 5890+-48 | log g : 3.9+-0.22 | vturb : 0.95+-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 | ... | ... | 2.21 | -1.05 | 0.45 | 2.21 | Li I |
CH | 1 | ... | -0.10+-0.25 | 6.92 | -1.51 | -0.01+-0.25 | 6.92 | CH |
CN | 1 | ... | 0.25+-0.28 | 6.67 | -1.16 | 0.34+-0.28 | 6.67 | CN |
O I | 2 | ... | 0.43+-0.19 | 7.62 | -1.07 | 0.43+-0.19 | 7.62 | O I |
Na I | 2 | ... | -0.02+-0.22 | 4.72 | -1.52 | -0.02+-0.22 | 4.72 | Na I |
Mg I | 3 | ... | 0.36+-0.23 | 6.46 | -1.14 | 0.36+-0.23 | 6.46 | Mg I |
Al I | 1 | ... | -0.32+-0.34 | 4.63 | -1.82 | -0.32+-0.34 | 4.63 | Al I |
Si I | 3 | ... | 0.45+-0.26 | 6.46 | -1.05 | 0.45+-0.26 | 6.46 | Si I |
K I | 1 | ... | 0.35+-0.25 | 3.88 | -1.15 | 0.35+-0.25 | 3.88 | K I |
Ca I | 12 | ... | 0.42+-0.27 | 5.26 | -1.08 | 0.42+-0.27 | 5.26 | Ca I |
Sc II | 6 | ... | 0.04+-0.14 | 1.76 | -1.39 | 0.11+-0.14 | 1.76 | Sc II |
Ti I | 15 | ... | 0.22+-0.20 | 3.67 | -1.28 | 0.22+-0.20 | 3.67 | Ti I |
Ti II | 24 | ... | 0.36+-0.13 | 3.88 | -1.07 | 0.43+-0.13 | 3.88 | Ti II |
V I | 1 | ... | 0.02+-0.22 | 2.45 | -1.48 | 0.02+-0.22 | 2.45 | V I |
V II | 2 | ... | 0.15+-0.23 | 2.65 | -1.28 | 0.22+-0.23 | 2.65 | V II |
Cr I | 10 | ... | -0.13+-0.20 | 4.01 | -1.63 | -0.13+-0.20 | 4.01 | Cr I |
Cr II | 3 | ... | 0.18+-0.14 | 4.38 | -1.26 | 0.24+-0.14 | 4.38 | Cr II |
Mn I | 4 | ... | -0.44+-0.20 | 3.50 | -1.93 | -0.43+-0.20 | 3.50 | Mn I |
Fe I | 112 | -1.50+-0.21 | ... | 6.00 | -1.50+-0.21 | ... | 6.00 | Fe I |
Fe II | 11 | -1.44+-0.14 | ... | 6.06 | -1.44+-0.14 | ... | 6.06 | Fe II |
Co I | 3 | ... | -0.11+-0.26 | 3.38 | -1.61 | -0.11+-0.26 | 3.38 | Co I |
Ni I | 10 | ... | 0.07+-0.22 | 4.79 | -1.43 | 0.07+-0.22 | 4.79 | Ni I |
Cu I | 1 | ... | -0.48+-0.22 | 2.21 | -1.98 | -0.48+-0.22 | 2.21 | Cu I |
Zn I | 3 | ... | 0.16+-0.20 | 3.22 | -1.34 | 0.16+-0.20 | 3.22 | Zn I |
Rb I | 1 | ... | <1.38 | <2.40 | <0.04 | <1.54 | <2.40 | Rb I |
Sr II | 1 | ... | 0.29+-0.13 | 1.72 | -1.15 | 0.35+-0.13 | 1.72 | Sr II |
Y II | 5 | ... | -0.06+-0.15 | 0.72 | -1.49 | 0.01+-0.15 | 0.72 | Y II |
Zr II | 3 | ... | 0.45+-0.14 | 1.59 | -0.99 | 0.51+-0.14 | 1.59 | Zr II |
Nb II | 1 | ... | <1.49 | <1.51 | <0.05 | <1.55 | <1.51 | Nb II |
Mo I | 1 | ... | <0.61 | <0.99 | <-0.89 | <0.61 | <0.99 | Mo I |
Tc I | 1 | ... | ... | <1.38 | <1.38 | <2.88 | <1.38 | Tc I |
Sn I | 1 | ... | <1.54 | <2.11 | <0.04 | <1.54 | <2.11 | Sn I |
Ba II | 3 | ... | 0.29+-0.13 | 1.04 | -1.14 | 0.36+-0.13 | 1.04 | Ba II |
La II | 4 | ... | 0.12+-0.16 | -0.22 | -1.32 | 0.18+-0.16 | -0.22 | La II |
Ce II | 4 | ... | 0.13+-0.20 | 0.28 | -1.30 | 0.20+-0.20 | 0.28 | Ce II |
Nd II | 1 | ... | -0.12+-0.18 | -0.14 | -1.56 | -0.06+-0.18 | -0.14 | Nd II |
Eu II | 2 | ... | 0.12+-0.14 | -0.80 | -1.32 | 0.18+-0.14 | -0.80 | Eu II |
Gd II | 1 | ... | <0.53 | <0.16 | <-0.91 | <0.59 | <0.16 | Gd II |
Tb II | 4 | ... | <0.95 | <-0.19 | <-0.51 | <0.99 | <-0.19 | Tb II |
Dy II | 1 | ... | <0.26 | <-0.08 | <-1.18 | <0.32 | <-0.08 | Dy II |
Er II | 1 | ... | <0.91 | <0.39 | <-0.53 | <0.97 | <0.39 | Er II |
Tm II | 1 | ... | <1.66 | <0.32 | <0.20 | <1.70 | <0.32 | Tm II |
Hf II | 2 | ... | <1.00 | <0.41 | <-0.30 | <1.20 | <0.41 | Hf II |
Pb I | 1 | ... | <1.29 | <1.83 | <-0.21 | <1.29 | <1.83 | Pb I |
Binary Parameters
Binarity | Negative |
Vrad | -94.4 |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-08-13-09:38 | 2454691.906 | MCDONALD | 33000 | 60-170 | 5400 | -94.3 |
2008-09-05-06:51 | 2454714.79 | MCDONALD | 33000 | 60-170 | 3600 | -94.6 |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 5974 | log g : 4.18 | 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 | -1.32 | ... | ... | -1.32 | ... | 6.18 | Fe |
Cu | N/A | ... | -0.41+-0.00 | ... | -1.71+-0.00 | -0.39+-0.00 | 2.48+-0.00 | Cu |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | 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 | 55000 | 250-500 | N/A | N/A |
Beryllium and Alpha-element Abundances in a Large Sample of Metal-poor Stars
Stellar Parameters
Teff : 5975+-100 | log g : 3.72+-0.2 | vturb : 1.31+-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 |
Be | N/A | ... | +0.15+-0.15 | +0.22+-0.12 | -1.16+-0.12 | 0.19+-0.15 | +0.22+-0.12 | Be |
O | N/A | -0.78+-0.22 | +0.57+-0.24 | ... | -0.84+-0.22 | 0.51+-0.24 | 7.85+-0.22 | O |
Mg | N/A | -0.97+-0.07 | ... | ... | -0.99+-0.07 | 0.36+-0.07 | 6.61+-0.07 | Mg |
Ti | N/A | -1.11+-0.09 | ... | ... | -1.04+-0.09 | 0.31+-0.09 | 3.91+-0.09 | Ti |
Fe | N/A | -1.35+-0.09 | ... | ... | -1.35+-0.09 | ... | 6.15+-0.09 | Fe |
Position
Right Ascension : | Declination : | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-19 | N/A | KECKHIRES | 42000 | 121 | 1800 | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5974 | log g : 4.18 | 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 | ... | -0.04 | ... | -1.27 | 0.05 | 4.97 | Na |
Mg | N/A | ... | 0.39 | ... | -0.95 | 0.37 | 6.65 | Mg |
Si | N/A | ... | 0.37 | ... | -0.91 | 0.41 | 6.60 | Si |
Ca | N/A | ... | 0.37 | ... | -0.93 | 0.39 | 5.41 | Ca |
Ti | N/A | ... | 0.28 | ... | -0.97 | 0.35 | 3.98 | Ti |
Cr | N/A | ... | -0.04 | ... | -1.33 | -0.01 | 4.31 | Cr |
Fe | N/A | -1.32 | ... | ... | -1.32 | ... | 6.18 | Fe |
Ni | N/A | ... | -0.01 | ... | -1.30 | 0.02 | 4.92 | Ni |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-09-0608 | N/A | VLT | 55000 | 450 | N/A | -93.9 |
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 | ... | -0.34 | ... | -1.70 | -0.38 | 3.73 | Mn |
Fe | N/A | -1.32 | ... | ... | -1.32 | ... | 6.18 | Fe |
Cu | N/A | ... | -0.41 | ... | -1.71 | -0.39 | 2.48 | Cu |
Zn | N/A | ... | 0.15 | ... | -1.13 | 0.19 | 3.43 | Zn |
Y | N/A | ... | 0.15 | ... | -1.14 | 0.18 | 1.07 | Y |
Ba | N/A | ... | 0.03 | ... | -1.34 | -0.02 | 0.84 | Ba |
Position
Right Ascension : 21 43 57.12 | Declination : +27 23 24.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-09-0608 | N/A | VLT | 55000 | 450 | N/A | -93.9 |