J0124+2508
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
Teff : 6545+-130 | log g : 4.15+-0.03 | vturb : 1.30+-0.30 |
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | 1 | ... | 2.11+-0.16 | 2.11+-0.16 | -1.15+-0.16 | 2.02+-0.16 | 2.11+-0.16 | Li I |
C | ... | <2.00 | <7.26 | <-1.17 | <2.00 | <7.26 | C | |
Mg I | 2 | ... | 0.22+-0.12 | 4.65+-0.12 | -2.95+-0.12 | 0.22+-0.12 | 4.65+-0.12 | Mg I |
Ca I | 2 | ... | 0.77+-0.15 | 3.94+-0.15 | -2.40+-0.15 | 0.77+-0.15 | 3.94+-0.15 | Ca I |
Sc II | 1 | ... | 0.26+-0.16 | 0.24+-0.16 | -2.91+-0.16 | 0.26+-0.16 | 0.24+-0.16 | Sc II |
Ti II | 6 | ... | 0.40+-0.13 | 2.18+-0.13 | -2.77+-0.13 | 0.40+-0.13 | 2.18+-0.13 | Ti II |
Cr I | 2 | ... | 0.15+-0.11 | 2.62+-0.11 | -3.02+-0.11 | 0.15+-0.11 | 2.62+-0.11 | Cr I |
Fe I | 13 | ... | 0.00+-0.16 | 4.33+-0.16 | -3.17+-0.16 | 0.00+-0.16 | 4.33+-0.16 | Fe I |
Fe II | 2 | ... | -0.28+-0.16 | 4.05+-0.16 | -3.45+-0.16 | -0.28+-0.16 | 4.05+-0.16 | Fe II |
Right Ascension : 01 24 54.99 | Declination : +25 08 21.21 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
N/A | N/A | SUBARUHDS | 36000 | 31.0 | N/A | 24.8 |