TYC22-155-1

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 : 4704+-9 log g : 3.10+-0.32 vturb : 1.04+-0.05

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-0.20+-0.10......-0.20+-0.10...7.30+-0.10Fe
Pr IIN/A...0.18+-0.120.70-0.020.18+-0.120.70Pr II
Nd IIN/A...0.28+-0.081.550.130.33+-0.081.55Nd II
Sm IIN/A...0.22+-0.050.980.020.22+-0.050.98Sm II
Eu IIN/A...0.48+-0.090.800.280.48+-0.090.80Eu 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