HR3018

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-0.82......-0.82...6.68Fe I
Fe IIN/A-0.91......-0.91...6.59Fe II
La IIN/A......0.36-0.740.080.36La II
Eu IIN/A......-0.03-0.550.27-0.03Eu 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...0.18...-0.510.275.73Na
MgN/A...0.38...-0.420.367.18Mg
CaN/A...0.26...-0.500.285.84Ca
TiN/A...0.14...-0.570.214.38Ti
FeN/A-0.78......-0.78...6.72Fe
NiN/A...-0.03...-0.780.005.44Ni
YN/A...0.01...-0.740.041.47Y
BaN/A...-0.24...-1.07-0.291.11Ba
EuN/A...0.4...-0.390.390.13Eu