J0759+5411

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 : 6493+-145 log g : 4.16+-0.05 vturb : 2.41+-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...<1.92<7.17<-1.26<1.94<7.17C
Na I1...-0.45+-0.162.61+-0.16-3.63+-0.16-0.43+-0.162.61+-0.16Na I
Mg I2...0.26+-0.124.68+-0.12-2.92+-0.120.28+-0.124.68+-0.12Mg I
Ti II3...0.44+-0.122.21+-0.12-2.74+-0.120.46+-0.122.21+-0.12Ti II
Fe I10...-0.02+-0.144.30+-0.14-3.20+-0.14-0.02+-0.144.30+-0.14Fe I
Fe II2...-0.37+-0.143.95+-0.14-3.55+-0.14-0.37+-0.143.95+-0.14Fe II

Position

Right Ascension : 07 59 00.25 Declination : +54 11 07.43 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 36.4 N/A 34.2