J1151-0054

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 : 6010+-100 log g : 3.61+-0.04 vturb : 0.00+-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
Li I1...1.85+-0.271.85+-0.27-1.41+-0.271.68+-0.271.85+-0.27Li I
C...<1.12<6.50<-1.93<1.16<6.50C
Mg I2...-0.25+-0.194.30+-0.19-3.30+-0.19-0.21+-0.194.30+-0.19Mg I
Ca I2...0.81+-0.194.10+-0.19-2.24+-0.190.85+-0.194.10+-0.19Ca I
Ti II1...0.01+-0.281.91+-0.28-3.04+-0.280.05+-0.281.91+-0.28Ti II
Cr I1...-0.31+-0.272.28+-0.27-3.36+-0.27-0.27+-0.272.28+-0.27Cr I
Fe I10...-0.04+-0.264.41+-0.26-3.09+-0.26-0.04+-0.264.41+-0.26Fe I
Fe II2...-0.46+-0.083.99+-0.08-3.51+-0.08-0.46+-0.083.99+-0.08Fe II

Position

Right Ascension : 11 51 14.97 Declination : -00 54 11.34 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 39.3 N/A -33.0