G95-57A

taken from 2 paper(s):

/J.Simmerer et al.(2004)/ /I.U.Roederer et al.(2010)/


J.Simmerer et al.,ApJ, 617, 1091, 2004(ADS)

The Rise of the s-Process in the Galaxy


Stellar Parameters

Teff : 4965 log g : 4.40 vturb : 0.90

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
CN/A...-0.05...-1.090.137.34C
Fe I17-1.22......-1.22...6.28Fe I
Fe II6-1.15......-1.15...6.35Fe II
La IIN/A......0.43+-0.09-0.67+-0.090.55+-0.090.43+-0.09La II
Eu IIN/A......-0.23+-0.1-0.75+-0.10.47+-0.1-0.23+-0.1Eu II

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A MCDONALD 60000 100 N/A N/A

I.U.Roederer et al.,ApJ, 724, 975, 2010(ADS)

THE UBIQUITY OF THE RAPID NEUTRON-CAPTURE PROCESS


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
FeN/A-1.22......-1.22...6.28Fe
Zn IN/A......3.70-0.860.363.70Zn I
Y IIN/A......1.34-0.870.351.34Y II
Pb IN/A......+1.14-0.900.32+1.14Pb I

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A MCDONALD 60000 100 N/A N/A