J1341+5135

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 : 6560+-160 log g : 4.32+-0.04 vturb : 0.27+-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
C...<2.00<7.41<-1.02<1.95<7.41C
Na I1...-0.59+-0.272.63+-0.27-3.61+-0.27-0.64+-0.272.63+-0.27Na I
Mg I2...0.24+-0.204.82+-0.20-2.78+-0.200.19+-0.204.82+-0.20Mg I
Ca I1...1.39+-0.274.71+-0.27-1.63+-0.271.34+-0.274.71+-0.27Ca I
Ti II1...1.01+-0.282.94+-0.28-2.01+-0.280.96+-0.282.94+-0.28Ti II
Fe I7...0.05+-0.254.53+-0.25-2.97+-0.250.05+-0.254.53+-0.25Fe I
Fe II1-0.70+-0.11...3.78+-0.11-3.72+-0.11...3.78+-0.11Fe II

Position

Right Ascension : 13 41 57.97 Declination : +51 35 34.09 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 28.0 N/A 45.0