G102-20

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 : 5254 log g : 4.44 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...-0.2...-1.27-0.027.16C
Fe I15-1.25......-1.25...6.25Fe I
Fe II7-1.21......-1.21...6.29Fe II
La IIN/A......-0.02+-0.12-1.12+-0.120.13+-0.12-0.02+-0.12La II
Eu IIN/A......-0.32+-0.06-0.84+-0.060.41+-0.06-0.32+-0.06Eu 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-1.25......-1.25...6.25Fe
Zn IN/A......3.47-1.090.163.47Zn I
Y IIN/A......0.78-1.43-0.180.78Y II
Pb IN/A......0.79-1.250.000.79Pb I

Position

Observing Log

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