J1127+1041

taken from 1 paper(s):

/H.Li et al.(2022)/


H.Li et al.,ApJ, 931, 147, 2022(ADS)

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances


Stellar Parameters

Teff : 6164+-175 log g : 4.47+-0.05 vturb : 1.50+-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
Na I1...0.09+-0.322.97+-0.32-3.27+-0.320.11+-0.322.97+-0.32Na I
Mg I2...0.36+-0.234.60+-0.23-3.00+-0.230.38+-0.234.60+-0.23Mg I
Ca I1...0.32+-0.323.30+-0.32-3.04+-0.320.34+-0.323.30+-0.32Ca I
Fe I4...-0.02+-0.374.12+-0.37-3.38+-0.37-0.02+-0.374.12+-0.37Fe I
Fe II1...0.35+-0.154.49+-0.15-3.01+-0.150.35+-0.154.49+-0.15Fe II

Position

Right Ascension : 11 27 25.19 Declination : +10 41 12.11 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 SUBARUHDS 36000 14.5 N/A -34.4