J2241+2924

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 : 6394+-225 log g : 4.07+-0.07 vturb : 3.10+-0.30

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
Mg I2...0.01+-0.093.88+-0.09-3.72+-0.090.01+-0.093.88+-0.09Mg I
Ca I1...-0.23+-0.102.38+-0.10-3.96+-0.10-0.23+-0.102.38+-0.10Ca I
Fe I10...0.00+-0.113.77+-0.11-3.73+-0.110.00+-0.113.77+-0.11Fe I
Fe II1...0.22+-0.173.99+-0.17-3.51+-0.170.22+-0.173.99+-0.17Fe II

Position

Right Ascension : 22 41 45.14 Declination : +29 24 28.14 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 34.9 N/A -216.9