G94-49

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 : 5373 log g : 4.5 vturb : 1.1

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...-0.650.155.59Na
MgN/A...0.34...-0.480.327.12Mg
SiN/A...0.32...-0.440.367.07Si
CaN/A...0.29...-0.490.315.85Ca
TiN/A...0.28...-0.450.354.50Ti
CrN/A...0.03...-0.740.064.90Cr
FeN/A-0.80......-0.80...6.70Fe
NiN/A...0.01...-0.760.045.46Ni

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 : 5373 log g : 4.5

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
MnN/A...-0.19...-1.03-0.234.40Mn
FeN/A-0.8......-0.80...6.70Fe
CuN/A...-0.05...-0.83-0.033.36Cu
ZnN/A...0.21...-0.550.254.01Zn
YN/A...0.02...-0.750.051.46Y
BaN/A...-0.14...-0.99-0.191.19Ba