G150-40

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 : 5968 log g : 4.09 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...0.28...-0.440.375.80Na
MgN/A...0.14...-0.690.126.91Mg
SiN/A...0.19...-0.580.236.93Si
CaN/A...0.19...-0.600.215.74Ca
TiN/A...0.12...-0.620.194.33Ti
CrN/A...0.01...-0.770.044.87Cr
FeN/A-0.81......-0.81...6.69Fe
NiN/A...-0.08...-0.86-0.055.36Ni

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 : 5968 log g : 4.09

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...-0.20...-1.05-0.244.38Mn
FeN/A-0.81......-0.81...6.69Fe
CuN/A...-0.28...-1.07-0.263.12Cu
ZnN/A...0.01...-0.760.053.80Zn
YN/A...-0.16...-0.94-0.131.27Y
BaN/A...-0.13...-0.99-0.181.19Ba