HR2906

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-0.18......-0.18...7.32Fe I
Fe IIN/A-0.21......-0.21...7.29Fe II
La IIN/A......0.92-0.18-0.000.92La 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...0.02...-0.070.116.17Na
MgN/A...0.09...-0.110.077.49Mg
CaN/A...0.02...-0.140.046.20Ca
TiN/A...0.04...-0.070.114.88Ti
FeN/A-0.18......-0.18...7.32Fe
NiN/A...-0.04...-0.19-0.016.03Ni
YN/A...0.17...0.020.202.23Y
BaN/A...0.1...-0.130.052.05Ba
EuN/A...0.15...-0.040.140.48Eu