J1458+1128
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
Teff : 5004+-64 | log g : 3.15+-0.30 | vturb : 1.37+-0.29 |
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 | ... | 0.57+-0.31 | 5.41+-0.31 | -3.02+-0.31 | 0.57+-0.31 | 5.41+-0.31 | C |
Na I | 2 | ... | -0.37+-0.15 | 2.28+-0.15 | -3.96+-0.15 | -0.37+-0.15 | 2.28+-0.15 | Na I |
Mg I | 2 | ... | -0.23+-0.16 | 3.78+-0.16 | -3.82+-0.16 | -0.23+-0.16 | 3.78+-0.16 | Mg I |
Ca I | 1 | ... | -1.06+-0.21 | 1.69+-0.21 | -4.65+-0.21 | -1.06+-0.21 | 1.69+-0.21 | Ca I |
Sc II | 1 | ... | 0.68+-0.25 | 0.24+-0.25 | -2.91+-0.25 | 0.68+-0.25 | 0.24+-0.25 | Sc II |
Ti II | 4 | ... | 0.34+-0.14 | 1.70+-0.14 | -3.25+-0.14 | 0.34+-0.14 | 1.70+-0.14 | Ti II |
Cr I | 1 | ... | -0.02+-0.21 | 2.03+-0.21 | -3.61+-0.21 | -0.02+-0.21 | 2.03+-0.21 | Cr I |
Fe I | 26 | ... | 0.00+-0.21 | 3.91+-0.21 | -3.59+-0.21 | 0.00+-0.21 | 3.91+-0.21 | Fe I |
Fe II | 2 | ... | 0.05+-0.14 | 3.96+-0.14 | -3.54+-0.14 | 0.05+-0.14 | 3.96+-0.14 | Fe II |
Sr II | 1 | ... | 0.45+-0.25 | -0.27+-0.25 | -3.14+-0.25 | 0.45+-0.25 | -0.27+-0.25 | Sr II |
Right Ascension : 14 58 22.30 | Declination : +11 28 14.30 | 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 | 23.5 | N/A | -8.8 |
N/A | N/A | SUBARUHDS | 36000 | 13.7 | N/A | 103.6 |