HR672

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-0.06......-0.06...7.44Fe I
Fe IIN/A-0.23......-0.23...7.27Fe II
La IIN/A......0.89-0.21-0.150.89La II
Eu IIN/A......0.3-0.22-0.160.3Eu II

Position

Right Ascension : 02 18 01.40 Declination : +01 45 28.0 Galactic Longitude (l) : N/A Galactic Latitude (b) : N/A

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...0.13...0.280.226.52Na
CaN/A...-0.01...0.070.016.41Ca
FeN/A0.06......0.06...7.56Fe
NiN/A...0.07...0.160.106.38Ni
YN/A...-0.06...0.03-0.032.24Y
BaN/A...-0.43...-0.42-0.481.76Ba
EuN/A...-0.07...-0.02-0.080.50Eu

Position

Right Ascension : 02 18 01.40 Declination : +01 45 28.0 Galactic Longitude (l) : N/A Galactic Latitude (b) : N/A

Observing Log