G161-73
taken from 3 paper(s):
/I.U.Roederer et al.(2014)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 5680+-49 | log g : 3.9+-0.22 | vturb : 1.05+-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 | ... | ... | 2.14 | -1.12 | 0.30 | 2.14 | Li I |
CH | 1 | ... | -0.63+-0.25 | 6.78 | -1.65 | -0.23+-0.25 | 6.78 | CH |
CN | 1 | ... | <0.64 | <7.45 | <-0.38 | <1.04 | <7.45 | CN |
O I | 3 | ... | 0.64+-0.19 | 7.90 | -0.79 | 0.63+-0.19 | 7.90 | O I |
Na I | 2 | ... | -0.14+-0.22 | 4.68 | -1.56 | -0.14+-0.22 | 4.68 | Na I |
Mg I | 3 | ... | 0.12+-0.23 | 6.30 | -1.30 | 0.12+-0.23 | 6.30 | Mg I |
Al I | 1 | ... | -0.97+-0.33 | 4.06 | -2.39 | -0.97+-0.33 | 4.06 | Al I |
Si I | 3 | ... | 0.21+-0.27 | 6.29 | -1.22 | 0.20+-0.27 | 6.29 | Si I |
K I | 2 | ... | 0.16+-0.25 | 3.76 | -1.27 | 0.15+-0.25 | 3.76 | K I |
Ca I | 8 | ... | 0.36+-0.29 | 5.27 | -1.07 | 0.35+-0.29 | 5.27 | Ca I |
Sc II | 6 | ... | -0.12+-0.13 | 1.96 | -1.19 | 0.23+-0.13 | 1.96 | Sc II |
Ti I | 11 | ... | 0.10+-0.20 | 3.62 | -1.33 | 0.09+-0.20 | 3.62 | Ti I |
Ti II | 20 | ... | 0.18+-0.14 | 4.07 | -0.88 | 0.54+-0.14 | 4.07 | Ti II |
V I | 1 | ... | -0.21+-0.22 | 2.30 | -1.63 | -0.21+-0.22 | 2.30 | V I |
V II | 2 | ... | 0.01+-0.23 | 2.87 | -1.06 | 0.36+-0.23 | 2.87 | V II |
Cr I | 9 | ... | -0.12+-0.20 | 4.10 | -1.54 | -0.12+-0.20 | 4.10 | Cr I |
Cr II | 3 | ... | 0.23+-0.14 | 4.80 | -0.84 | 0.58+-0.14 | 4.80 | Cr II |
Mn I | 4 | ... | -0.31+-0.22 | 3.69 | -1.74 | -0.32+-0.22 | 3.69 | Mn I |
Fe I | 94 | -1.42+-0.22 | ... | 6.08 | -1.42+-0.22 | ... | 6.08 | Fe I |
Fe II | 10 | -1.07+-0.15 | ... | 6.43 | -1.07+-0.15 | ... | 6.43 | Fe II |
Co I | 3 | ... | -0.44+-0.26 | 3.12 | -1.87 | -0.45+-0.26 | 3.12 | Co I |
Ni I | 7 | ... | -0.01+-0.22 | 4.79 | -1.43 | -0.01+-0.22 | 4.79 | Ni I |
Zn I | 2 | ... | 0.08+-0.19 | 3.22 | -1.34 | 0.08+-0.19 | 3.22 | Zn I |
Sr II | 2 | ... | -0.25+-0.14 | 1.55 | -1.32 | 0.10+-0.14 | 1.55 | Sr II |
Y II | 3 | ... | -0.42+-0.14 | 0.73 | -1.48 | -0.06+-0.14 | 0.73 | Y II |
Zr II | 3 | ... | 0.05+-0.14 | 1.57 | -1.01 | 0.41+-0.14 | 1.57 | Zr II |
Nb II | 1 | ... | <1.43 | <1.82 | <0.36 | <1.78 | <1.82 | Nb II |
Mo I | 1 | ... | <0.53 | <0.99 | <-0.89 | <0.53 | <0.99 | Mo I |
Tc I | 1 | ... | ... | <1.10 | <1.10 | <2.52 | <1.10 | Tc I |
Ba II | 3 | ... | -0.06+-0.13 | 1.05 | -1.13 | 0.29+-0.13 | 1.05 | Ba II |
La II | 3 | ... | -0.14+-0.15 | -0.10 | -1.20 | 0.22+-0.15 | -0.10 | La II |
Ce II | 2 | ... | -0.10+-0.19 | 0.41 | -1.17 | 0.25+-0.19 | 0.41 | Ce II |
Nd II | 3 | ... | 0.00+-0.16 | 0.35 | -1.07 | 0.35+-0.16 | 0.35 | Nd II |
Eu II | 2 | ... | 0.03+-0.13 | -0.52 | -1.04 | 0.38+-0.13 | -0.52 | Eu II |
Gd II | 1 | ... | 0.31+-0.22 | 0.31 | -0.76 | 0.66+-0.22 | 0.31 | Gd II |
Er II | 2 | ... | <0.33 | <0.18 | <-0.74 | <0.68 | <0.18 | Er II |
Tm II | 2 | ... | <0.36 | <-0.61 | <-0.73 | <0.69 | <-0.61 | Tm II |
Hf II | 2 | ... | <0.89 | <0.67 | <-0.04 | <1.38 | <0.67 | Hf II |
Pb I | 1 | ... | <0.84 | <1.46 | <-0.58 | <0.84 | <1.46 | Pb I |
Th II | 1 | ... | <1.54 | <0.53 | <0.47 | <1.89 | <0.53 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | 121.1 |
Position
Right Ascension : 09 45 37.82 | Declination : -04 40 28.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2009-02-19-03:44 | 2454881.661 | MCDONALD | 33000 | 30-100 | 7200 | 121.3 |
2009-02-19-06:00 | 2454881.755 | MCDONALD | 33000 | 30-100 | 7200 | 121 |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5986 | log g : 4 | vturb : 1.4 |
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 | ... | -0.36 | ... | -1.27 | -0.27 | 4.97 | Na |
Mg | N/A | ... | 0.13 | ... | -0.89 | 0.11 | 6.71 | Mg |
Si | N/A | ... | 0.13 | ... | -0.83 | 0.17 | 6.68 | Si |
Ca | N/A | ... | 0.25 | ... | -0.73 | 0.27 | 5.61 | Ca |
Ti | N/A | ... | 0.14 | ... | -0.79 | 0.21 | 4.16 | Ti |
Cr | N/A | ... | -0.06 | ... | -1.03 | -0.03 | 4.61 | Cr |
Fe | N/A | -1.00 | ... | ... | -1.00 | ... | 6.50 | Fe |
Ni | N/A | ... | -0.15 | ... | -1.12 | -0.12 | 5.10 | Ni |
Position
Right Ascension : 09 45 37.82 | Declination : -04 40 28.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-20-2156 | N/A | FIESNOT | 40000 | 155 | N/A | 121.2 |
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 | ... | -0.36 | ... | -1.40 | -0.40 | 4.03 | Mn |
Fe | N/A | -1 | ... | ... | -1.00 | ... | 6.50 | Fe |
Zn | N/A | ... | -0.08 | ... | -1.04 | -0.04 | 3.52 | Zn |
Y | N/A | ... | -0.19 | ... | -1.16 | -0.16 | 1.05 | Y |
Ba | N/A | ... | -0.11 | ... | -1.16 | -0.16 | 1.02 | Ba |
Position
Right Ascension : 09 45 37.82 | Declination : -04 40 28.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-20-2156 | N/A | FIESNOT | 40000 | 155 | N/A | 121.2 |