HE1320+0038
/J.G.Cohen et al.(2004)/ /J.G.Cohen et al.(2013)/
Abundances In Very Metal-Poor Dwarf Stars
Teff : 6500 | log g : 3.7 | vturb : 1.9 |
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 | 4 | ... | ... | 5.40+-0.19 | -2.20+-0.19 | 0.51+-0.19 | 5.40+-0.19 | Mg I |
Al I | 2 | ... | ... | 3.70+-0.03 | -2.75+-0.03 | -0.04+-0.03 | 3.70+-0.03 | Al I |
Si I | 1 | ... | ... | 4.77 | -2.74 | -0.03 | 4.77 | Si I |
Ca I | 5 | ... | ... | 3.98+-0.12 | -2.36+-0.12 | 0.35+-0.12 | 3.98+-0.12 | Ca I |
Sc II | 2 | ... | ... | 0.48+-0.02 | -2.67+-0.02 | 0.04+-0.02 | 0.48+-0.02 | Sc II |
Ti I | 1 | ... | ... | <2.98 | <-1.97 | <0.74 | <2.98 | Ti I |
Ti II | 12 | ... | ... | 2.61+-0.05 | -2.34+-0.05 | 0.37+-0.05 | 2.61+-0.05 | Ti II |
Cr I | 4 | ... | ... | 2.80+-0.07 | -2.84+-0.07 | -0.13+-0.07 | 2.80+-0.07 | Cr I |
Mn I | 2 | ... | ... | 2.17+-0.14 | -3.26+-0.14 | -0.55+-0.14 | 2.17+-0.14 | Mn I |
Fe I | 41 | ... | ... | 4.79+-0.15 | -2.71+-0.15 | ... | 4.79+-0.15 | Fe I |
Fe II | 7 | ... | ... | 4.83+-0.14 | -2.67+-0.14 | ... | 4.83+-0.14 | Fe II |
Co I | 2 | ... | ... | 2.62+-0.07 | -2.37+-0.07 | 0.34+-0.07 | 2.62+-0.07 | Co I |
Ni I | 1 | ... | ... | 3.54 | -2.68 | 0.03 | 3.54 | Ni I |
Sr II | 2 | ... | ... | -0.42+-0.04 | -3.29+-0.04 | -0.58+-0.04 | -0.42+-0.04 | Sr II |
Ba II | 2 | ... | ... | -1.06+-0.25 | -3.24+-0.25 | -0.53+-0.25 | -1.06+-0.25 | Ba II |
Eu II | 1 | ... | ... | <-0.72 | <-1.24 | <1.47 | <-0.72 | Eu II |
Right Ascension : 13 22 35.30 | Declination : +00 22 31.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2002-05 | N/A | KECKHIRES | 45000 | 100 | 2700 | N/A |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Teff : 6500+-100 | log g : 3.7+-0.25 | vturb : 1.9+-0.2 |
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 | 4 | ... | 0.41+-0.05 | ... | -2.31+-0.05 | 0.40+-0.05 | 5.29+-0.05 | Mg I |
Al I | 2 | ... | -0.1+-0.03 | ... | -2.74+-0.03 | -0.03+-0.03 | 3.71+-0.03 | Al I |
Si I | 1 | ... | -0.17 | ... | -2.79 | -0.08 | 4.72 | Si I |
Ca I | 5 | ... | 0.29+-0.12 | ... | -2.35+-0.12 | 0.36+-0.12 | 3.99+-0.12 | Ca I |
Sc II | 2 | ... | 0.05+-0.02 | ... | -2.66+-0.02 | 0.05+-0.02 | 0.49+-0.02 | Sc II |
Ti I | 1 | ... | <0.65 | ... | <-1.97 | <0.74 | <2.98 | Ti I |
Ti II | 12 | ... | 0.28+-0.05 | ... | -2.34+-0.05 | 0.37+-0.05 | 2.61+-0.05 | Ti II |
Cr I | 4 | ... | -0.21+-0.07 | ... | -2.84+-0.07 | -0.13+-0.07 | 2.80+-0.07 | Cr I |
Mn I | 2 | ... | -0.55+-0.14 | ... | -3.25+-0.14 | -0.54+-0.14 | 2.18+-0.14 | Mn I |
Fe I | N/A | -2.66+-0.14 | ... | ... | -2.71+-0.14 | ... | 4.79+-0.14 | Fe I |
Fe II | 7 | -2.62+-0.14 | 0.04+-0.14 | ... | -2.67+-0.14 | 0.04+-0.14 | 4.83+-0.14 | Fe II |
Co I | 2 | ... | 0.36+-0.07 | ... | -2.37+-0.07 | 0.34+-0.07 | 2.62+-0.07 | Co I |
Ni I | 1 | ... | -0.05 | ... | -2.68 | 0.03 | 3.54 | Ni I |
Sr II | 2 | ... | -0.66+-0.04 | ... | -3.29+-0.04 | -0.58+-0.04 | -0.42+-0.04 | Sr II |
Ba II | 1 | ... | -0.69 | ... | -3.40 | -0.69 | -1.22 | Ba II |
Eu II | 1 | ... | <1.43 | ... | <-1.24 | <1.47 | <-0.72 | Eu II |
Vrad | 22 |
Right Ascension : 13 22 35.30 | Declination : +00 22 31.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2002-05 | N/A | KECKHIRES | 36000 | 80 | 4100 | 22 |