HR1101

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-0.15......-0.15...7.35Fe I
Fe IIN/A-0.24......-0.24...7.26Fe II
La IIN/A......0.82-0.28-0.130.82La II
Eu IIN/A......0.24-0.28-0.130.24Eu 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...0.06...0.040.156.28Na
MgN/A...0.09...-0.040.077.56Mg
TiN/A...0.01...-0.030.084.92Ti
FeN/A-0.11......-0.11...7.39Fe
NiN/A...0.03...-0.050.066.17Ni
YN/A...-0.05...-0.13-0.022.08Y
BaN/A...-0.25...-0.41-0.301.77Ba
EuN/A...0.06...-0.060.050.46Eu