HR5235

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/A0.15......0.15...7.65Fe I
Fe IIN/A-0.41......-0.41...7.09Fe II
La IIN/A......1-0.10-0.251La II
Eu IIN/A......0.46-0.06-0.210.46Eu 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...0.26...0.540.356.78Na
MgN/A...0.28...0.450.268.05Mg
CaN/A...0.04...0.250.066.59Ca
TiN/A...0.13...0.390.205.34Ti
FeN/A0.19......0.19...7.69Fe
NiN/A...0.11...0.330.146.55Ni
BaN/A...-0.34...-0.20-0.391.98Ba