HR1729

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-0.14......-0.14...7.36Fe I
Fe IIN/A-0.29......-0.29...7.21Fe II
La IIN/A......0.89-0.21-0.070.89La II
Eu IIN/A......0.32-0.20-0.060.32Eu 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...0.07...0.130.166.37Na
MgN/A...0.13...0.080.117.68Mg
CaN/A...-0.01...-0.020.016.32Ca
TiN/A...0.05...0.090.125.04Ti
FeN/A-0.03......-0.03...7.47Fe
NiN/A...0.02...0.020.056.24Ni
YN/A...-0.29...-0.29-0.261.92Y
BaN/A...-0.38...-0.46-0.431.72Ba