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)/

I.U.Roederer et al.,AJ, 147, 136, 2014 (A0309,ADS)
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 |
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 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P.E.Nissen et al.,AAP, 511, L10, 2010 (C0012,ADS)
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 |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P. E. Nissen et al.,AAP, 530, A15, 2011 (C0013,ADS)
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 |