HIP108200
/E.M.O'Malley et al.(2017)/ /K.A.Venn et al.(2004)/
A Differential Abundance Analysis of Very Metal-poor Stars
Teff : 5175 | log g : 4.60 | vturb : 1.50 |
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Mg I | N/A | ... | 0.05+-0.15 | ... | -1.80+-0.15 | 0.03+-0.15 | 5.80+-0.15 | Mg I |
Ca I | N/A | ... | 0.14+-0.04 | ... | -1.67+-0.04 | 0.16+-0.04 | 4.67+-0.04 | Ca I |
Fe I | N/A | -1.83+-0.07 | ... | ... | -1.83+-0.07 | ... | 5.67+-0.07 | Fe I |
Fe II | N/A | -1.79+-0.18 | ... | ... | -1.79+-0.18 | ... | 5.71+-0.18 | Fe II |
Vrad | -184.2 |
Right Ascension : 21 55 16.10 | Declination : +32 38 41.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2012-08-14 | N/A | MIKELCO | 55000 | 92.17 | N/A | -184.2 |
Stellar Chemical Signatures and Hierarchical Galaxy Formation
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na | N/A | ... | -0.23 | ... | -2.04 | -0.14 | 4.20 | Na |
Mg | N/A | ... | 0.34 | ... | -1.58 | 0.32 | 6.02 | Mg |
Ca | N/A | ... | 0.2 | ... | -1.68 | 0.22 | 4.66 | Ca |
Ti | N/A | ... | 0.18 | ... | -1.65 | 0.25 | 3.30 | Ti |
Fe | N/A | -1.9 | ... | ... | -1.90 | ... | 5.60 | Fe |
Ni | N/A | ... | -0.09 | ... | -1.96 | -0.06 | 4.26 | Ni |
Y | N/A | ... | -0.24 | ... | -2.11 | -0.21 | 0.10 | Y |
Ba | N/A | ... | -0.07 | ... | -2.02 | -0.12 | 0.16 | Ba |
Right Ascension : 21 55 16.10 | Declination : +32 38 41.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |