J1614+5137

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+-101 log g : 4.06+-0.03 vturb : 1.88+-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
Na I2...-0.43+-0.112.90+-0.11-3.34+-0.11-0.42+-0.112.90+-0.11Na I
Mg I3...0.22+-0.134.91+-0.13-2.69+-0.130.23+-0.134.91+-0.13Mg I
Ca I2...0.56+-0.113.99+-0.11-2.35+-0.110.57+-0.113.99+-0.11Ca I
Ti II7...0.46+-0.132.50+-0.13-2.45+-0.130.47+-0.132.50+-0.13Ti II
Fe I11...-0.01+-0.144.58+-0.14-2.92+-0.14-0.01+-0.144.58+-0.14Fe I
Fe II2...-0.36+-0.084.23+-0.08-3.27+-0.08-0.36+-0.084.23+-0.08Fe II
Sr II2...0.10+-0.110.06+-0.11-2.81+-0.110.11+-0.110.06+-0.11Sr II
Ba II2...0.12+-0.11-0.61+-0.11-2.79+-0.110.13+-0.11-0.61+-0.11Ba II

Position

Right Ascension : 16 14 24.48 Declination : +51 37 12.77 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 42.2 N/A 20.9