HR3262

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-0.27......-0.27...7.23Fe I
Fe IIN/A-0.32......-0.32...7.18Fe II
La IIN/A......0.83-0.27-0.000.83La II
Eu IIN/A......0.32-0.200.070.32Eu 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...0.07...-0.100.166.14Na
CaN/A...0.03...-0.210.056.13Ca
TiN/A...0.14...-0.050.214.90Ti
FeN/A-0.26......-0.26...7.24Fe
NiN/A...-0.01...-0.240.025.98Ni
YN/A...0.01...-0.220.041.99Y
BaN/A...-0.08...-0.39-0.131.79Ba