G56-36

taken from 2 paper(s):

/P.E.Nissen and W. J. Schuster(2010)/ /P. E. Nissen and W. J. Schuster(2011)/


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 : 5933 log g : 4.28 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
NaN/A...-0.06...-0.910.035.33Na
MgN/A...0.19...-0.770.176.83Mg
SiN/A...0.19...-0.710.236.80Si
CaN/A...0.25...-0.670.275.67Ca
TiN/A...0.17...-0.700.244.25Ti
CrN/A...-0.02...-0.930.014.71Cr
FeN/A-0.94......-0.94...6.56Fe
NiN/A...-0.08...-0.99-0.055.23Ni

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

Teff : 5933 log g : 4.28

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
MnN/A...-0.27...-1.25-0.314.18Mn
FeN/A-0.94......-0.94...6.56Fe
CuN/A...-0.31...-1.23-0.292.96Cu
ZnN/A...0.01...-0.890.053.67Zn
YN/A...-0.05...-0.96-0.021.25Y
BaN/A...-0.02...-1.01-0.071.17Ba