HR1673

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-0.43......-0.43...7.07Fe I
Fe IIN/A-0.41......-0.41...7.09Fe II
La IIN/A......0.82-0.280.150.82La II
Eu IIN/A......0.13-0.390.040.13Eu 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...0.04...-0.170.136.07Na
MgN/A...0.16...-0.160.147.44Mg
CaN/A...0.07...-0.210.096.13Ca
TiN/A...0.19...-0.040.264.91Ti
FeN/A-0.3......-0.30...7.20Fe
NiN/A...0.11...-0.160.146.06Ni
YN/A...0.05...-0.220.081.99Y
BaN/A...-0.12...-0.47-0.171.71Ba
EuN/A...0.17...-0.140.160.38Eu