G18-28

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 : 5372 log g : 4.41 vturb : 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...-0.680.155.56Na
MgN/A...0.36...-0.490.347.11Mg
SiN/A...0.3...-0.490.347.02Si
CaN/A...0.29...-0.520.315.82Ca
TiN/A...0.27...-0.490.344.46Ti
CrN/A...0.05...-0.750.084.89Cr
FeN/A-0.83......-0.83...6.67Fe
NiN/A...0.00...-0.800.035.42Ni

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2005-10-13-0013 N/A VLT 55000 300 N/A -203.1
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 : 5372 log g : 4.41

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...-0.22...-1.09-0.264.34Mn
FeN/A-0.83......-0.83...6.67Fe
CuN/A...-0.09...-0.90-0.073.29Cu
ZnN/A...0.17...-0.620.213.94Zn
YN/A...0.04...-0.760.071.45Y
BaN/A...-0.07...-0.95-0.121.23Ba

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2005-10-13-0013 N/A VLT 55000 300 N/A -203.1