HE0458-1346
/J.G.Cohen et al.(2004)/ /J.G.Cohen et al.(2013)/
Abundances In Very Metal-Poor Dwarf Stars
Teff : 6210 | log g : 4.5 | vturb : 1.6 |
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 | 5 | ... | ... | 5.65+-0.31 | -1.95+-0.31 | 0.47+-0.31 | 5.65+-0.31 | Mg I |
Al I | 2 | ... | ... | 4.06+-0.14 | -2.39+-0.14 | 0.03+-0.14 | 4.06+-0.14 | Al I |
Si I | 1 | ... | ... | 5.43 | -2.08 | 0.34 | 5.43 | Si I |
Ca I | 6 | ... | ... | 4.19+-0.17 | -2.15+-0.17 | 0.27+-0.17 | 4.19+-0.17 | Ca I |
Sc II | 3 | ... | ... | 0.92+-0.05 | -2.23+-0.05 | 0.19+-0.05 | 0.92+-0.05 | Sc II |
Ti I | 6 | ... | ... | 3.06+-0.18 | -1.89+-0.18 | 0.53+-0.18 | 3.06+-0.18 | Ti I |
Ti II | 13 | ... | ... | 3.00+-0.11 | -1.95+-0.11 | 0.47+-0.11 | 3.00+-0.11 | Ti II |
Cr I | 4 | ... | ... | 3.03+-0.08 | -2.61+-0.08 | -0.19+-0.08 | 3.03+-0.08 | Cr I |
Mn I | 2 | ... | ... | 2.32+-0.22 | -3.11+-0.22 | -0.69+-0.22 | 2.32+-0.22 | Mn I |
Fe I | 61 | ... | ... | 5.08+-0.18 | -2.42+-0.18 | ... | 5.08+-0.18 | Fe I |
Fe II | 7 | ... | ... | 5.04+-0.18 | -2.46+-0.18 | ... | 5.04+-0.18 | Fe II |
Co I | 4 | ... | ... | 3.01+-0.28 | -1.98+-0.28 | 0.44+-0.28 | 3.01+-0.28 | Co I |
Ni I | 1 | ... | ... | 3.80 | -2.42 | 0.00 | 3.80 | Ni I |
Sr II | 2 | ... | ... | 0.59+-0.10 | -2.28+-0.10 | 0.14+-0.10 | 0.59+-0.10 | Sr II |
Ba II | 2 | ... | ... | -0.19+-0.04 | -2.37+-0.04 | 0.05+-0.04 | -0.19+-0.04 | Ba II |
Eu II | 1 | ... | ... | <-0.51 | <-1.03 | <1.39 | <-0.51 | Eu II |
Binarity | Positive |
Right Ascension : 05 01 11.70 | Declination : -13 42 40.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2002-09 | N/A | KECKHIRES | 34000 | 95 | 4800 | N/A |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Teff : 6210+-100 | log g : 4.5+-0.25 | vturb : 1.3+-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 | 5 | ... | 0.34+-0.18 | ... | -2.01+-0.18 | 0.33+-0.18 | 5.59+-0.18 | Mg I |
Al I | 2 | ... | -0.06+-0.14 | ... | -2.33+-0.14 | 0.01+-0.14 | 4.12+-0.14 | Al I |
Si I | 1 | ... | 0.17 | ... | -2.08 | 0.26 | 5.43 | Si I |
Ca I | 6 | ... | 0.15+-0.11 | ... | -2.12+-0.11 | 0.22+-0.11 | 4.22+-0.11 | Ca I |
Sc II | 3 | ... | 0.15+-0.05 | ... | -2.19+-0.05 | 0.15+-0.05 | 0.96+-0.05 | Sc II |
Ti I | 5 | ... | 0.32+-0.14 | ... | -1.93+-0.14 | 0.41+-0.14 | 3.02+-0.14 | Ti I |
Ti II | 13 | ... | 0.36+-0.11 | ... | -1.89+-0.11 | 0.45+-0.11 | 3.06+-0.11 | Ti II |
Cr I | 4 | ... | -0.28+-0.08 | ... | -2.54+-0.08 | -0.20+-0.08 | 3.10+-0.08 | Cr I |
Mn I | 2 | ... | -0.73+-0.16 | ... | -3.06+-0.16 | -0.72+-0.16 | 2.37+-0.16 | Mn I |
Fe I | N/A | -2.29+-0.14 | ... | ... | -2.34+-0.14 | ... | 5.16+-0.14 | Fe I |
Fe II | 7 | -2.35+-0.18 | -0.06+-0.18 | ... | -2.40+-0.18 | -0.06+-0.18 | 5.10+-0.18 | Fe II |
Co I | 4 | ... | 0.39+-0.28 | ... | -1.97+-0.28 | 0.37+-0.28 | 3.02+-0.28 | Co I |
Ni I | 1 | ... | -0.16 | ... | -2.42 | -0.08 | 3.80 | Ni I |
Sr II | 2 | ... | 0.15+-0.05 | ... | -2.11+-0.05 | 0.23+-0.05 | 0.76+-0.05 | Sr II |
Ba II | 1 | ... | 0.06 | ... | -2.28 | 0.06 | -0.10 | Ba II |
Eu II | 1 | ... | <1.28 | ... | <-1.02 | <1.32 | <-0.50 | Eu II |
Vrad | 359.4 |
Right Ascension : 05 01 11.70 | Declination : -13 42 40.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2002-09 | N/A | KECKHIRES | 36000 | 70 | 4800 | 359.4 |