BD+44_575

taken from 1 paper(s):

/D.Karinkuzhi et al.(2023)/


D.Karinkuzhi et al.,AAP, 677, A47, 2023(ADS)

Does the i-process operate at nearly solar metallicity?


Stellar Parameters

Teff : 4175+-6 log g : 1.50+-0.19 vturb : 1.60+-0.10

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-0.45+-0.05......-0.45+-0.05...7.05+-0.05Fe
Pr IIN/A...0.43+-0.140.70-0.020.43+-0.140.70Pr II
Nd IIN/A...0.45+-0.081.420.000.45+-0.081.42Nd II
Sm IIN/A...0.45+-0.050.960.000.45+-0.050.96Sm II
Eu IIN/A...0.43+-0.090.50-0.020.43+-0.090.50Eu II

Position

Right Ascension : Declination : 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 N/A HERMES 86000 N/A N/A N/A