HR2883

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-0.77......-0.77...6.73Fe I
Fe IIN/A-0.83......-0.83...6.67Fe II
La IIN/A......0.38-0.720.050.38La II
Eu IIN/A......-0.03-0.550.22-0.03Eu 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...0.03...-0.630.125.61Na
MgN/A...0.29...-0.480.277.12Mg
CaN/A...0.17...-0.560.195.78Ca
TiN/A...0.21...-0.470.284.48Ti
FeN/A-0.75......-0.75...6.75Fe
NiN/A...0.03...-0.690.065.53Ni
YN/A...0.01...-0.710.041.50Y
BaN/A...-0.23...-1.03-0.281.15Ba
EuN/A...0.31...-0.450.300.07Eu