HR2530

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-0.49......-0.49...7.01Fe I
Fe IIN/A-0.6......-0.60...6.90Fe II
La IIN/A......0.56-0.54-0.050.56La II
Eu IIN/A......0.12-0.400.090.12Eu 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...0.12...-0.220.216.02Na
CaN/A...0.04...-0.370.065.97Ca
FeN/A-0.43......-0.43...7.07Fe
NiN/A...0.02...-0.380.055.84Ni
YN/A...0.13...-0.270.161.94Y
EuN/A...0.06...-0.380.050.14Eu