HR3578

taken from 2 paper(s):

/J.Simmerer et al.(2004)/ /K.A.Venn et al.(2004)/


J.Simmerer et al.,ApJ, 617, 1091, 2004(ADS)

The Rise of the s-Process in the Galaxy


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
Fe IN/A-0.89......-0.89...6.61Fe I
Fe IIN/A-1......-1.00...6.50Fe II
La IIN/A......0.36-0.740.150.36La II
Eu IIN/A......-0.03-0.550.34-0.03Eu II

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A MCDONALD 60000 100 N/A N/A

K.A.Venn et al.,AJ, 128, 1177, 2004(ADS)

Stellar Chemical Signatures and Hierarchical Galaxy Formation


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...0.05...-0.680.145.56Na
MgN/A...0.35...-0.490.337.11Mg
CaN/A...0.23...-0.570.255.77Ca
TiN/A...0.26...-0.490.334.46Ti
FeN/A-0.82......-0.82...6.68Fe
NiN/A...0.01...-0.780.045.44Ni
YN/A...0.16...-0.630.191.58Y
BaN/A...-0.16...-1.03-0.211.15Ba
EuN/A...0.42...-0.410.410.11Eu