HE1141-0610
/J.G.Cohen et al.(2004)/ /J.G.Cohen et al.(2013)/
Abundances In Very Metal-Poor Dwarf Stars
Teff : 6730 | log g : 4.0 | 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 | 5 | ... | ... | 5.82+-0.13 | -1.78+-0.13 | 0.51+-0.13 | 5.82+-0.13 | Mg I |
Al I | 2 | ... | ... | 4.03+-0.19 | -2.42+-0.19 | -0.13+-0.19 | 4.03+-0.19 | Al I |
Si I | 1 | ... | ... | 5.04 | -2.47 | -0.18 | 5.04 | Si I |
Ca I | 7 | ... | ... | 4.33+-0.08 | -2.01+-0.08 | 0.28+-0.08 | 4.33+-0.08 | Ca I |
Sc II | 3 | ... | ... | 1.11+-0.12 | -2.04+-0.12 | 0.25+-0.12 | 1.11+-0.12 | Sc II |
Ti I | 5 | ... | ... | 3.16+-0.17 | -1.79+-0.17 | 0.50+-0.17 | 3.16+-0.17 | Ti I |
Ti II | 16 | ... | ... | 3.14+-0.09 | -1.81+-0.09 | 0.48+-0.09 | 3.14+-0.09 | Ti II |
V I | 1 | ... | ... | <2.60 | <-1.33 | <0.96 | <2.60 | V I |
Cr I | 4 | ... | ... | 3.24+-0.13 | -2.40+-0.13 | -0.11+-0.13 | 3.24+-0.13 | Cr I |
Mn I | 2 | ... | ... | 2.55+-0.01 | -2.88+-0.01 | -0.59+-0.01 | 2.55+-0.01 | Mn I |
Fe I | 47 | ... | ... | 5.21+-0.18 | -2.29+-0.18 | ... | 5.21+-0.18 | Fe I |
Fe II | 9 | ... | ... | 5.26+-0.16 | -2.24+-0.16 | ... | 5.26+-0.16 | Fe II |
Co I | 2 | ... | ... | 3.05+-0.25 | -1.94+-0.25 | 0.35+-0.25 | 3.05+-0.25 | Co I |
Ni I | 1 | ... | ... | 4.00 | -2.22 | 0.07 | 4.00 | Ni I |
Sr II | 2 | ... | ... | 0.67+-0.04 | -2.20+-0.04 | 0.09+-0.04 | 0.67+-0.04 | Sr II |
Ba II | 2 | ... | ... | -0.13+-0.01 | -2.31+-0.01 | -0.02+-0.01 | -0.13+-0.01 | Ba II |
Eu II | 1 | ... | ... | <-0.71 | <-1.23 | <1.06 | <-0.71 | Eu II |
Right Ascension : 11 44 22.60 | Declination : -06 26 59.0 | 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 : 6750+-100 | log g : 4.1+-0.25 | vturb : 2.1+-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 |
CH | N/A | ... | 0.89 | ... | -1.23 | 1.10 | 7.20 | CH |
O I | 3 | ... | 0.8+-0.04 | ... | -1.24+-0.04 | 1.09+-0.04 | 7.45+-0.04 | O I |
Na I | 2 | ... | -0.07+-0.11 | ... | -2.27+-0.11 | 0.06+-0.11 | 3.97+-0.11 | Na I |
Mg I | 5 | ... | 0.43+-0.07 | ... | -1.91+-0.07 | 0.42+-0.07 | 5.69+-0.07 | Mg I |
Al I | 2 | ... | -0.15+-0.17 | ... | -2.41+-0.17 | -0.08+-0.17 | 4.04+-0.17 | Al I |
Si I | 1 | ... | -0.32 | ... | -2.56 | -0.23 | 4.95 | Si I |
K I | 1 | ... | 0.33 | ... | -1.86 | 0.47 | 3.17 | K I |
Ca I | 8 | ... | 0.24+-0.06 | ... | -2.02+-0.06 | 0.31+-0.06 | 4.32+-0.06 | Ca I |
Sc II | 3 | ... | 0.32+-0.12 | ... | -2.01+-0.12 | 0.32+-0.12 | 1.14+-0.12 | Sc II |
Ti I | 5 | ... | 0.47+-0.17 | ... | -1.77+-0.17 | 0.56+-0.17 | 3.18+-0.17 | Ti I |
Ti II | 16 | ... | 0.44+-0.08 | ... | -1.80+-0.08 | 0.53+-0.08 | 3.15+-0.08 | Ti II |
V I | 1 | ... | 0.9 | ... | -1.31 | 1.02 | 2.62 | V I |
Cr I | 4 | ... | -0.15+-0.12 | ... | -2.40+-0.12 | -0.07+-0.12 | 3.24+-0.12 | Cr I |
Mn I | 2 | ... | -0.55+-0.01 | ... | -2.87+-0.01 | -0.54+-0.01 | 2.56+-0.01 | Mn I |
Fe I | N/A | -2.28+-0.17 | ... | ... | -2.33+-0.17 | ... | 5.17+-0.17 | Fe I |
Fe II | 9 | -2.17+-0.16 | 0.11+-0.16 | ... | -2.22+-0.16 | 0.11+-0.16 | 5.28+-0.16 | Fe II |
Co I | 2 | ... | 0.31+-0.23 | ... | -2.04+-0.23 | 0.29+-0.23 | 2.95+-0.23 | Co I |
Ni I | 1 | ... | -0.06 | ... | -2.31 | 0.02 | 3.91 | Ni I |
Sr II | 2 | ... | -0.03+-0.01 | ... | -2.28+-0.01 | 0.05+-0.01 | 0.59+-0.01 | Sr II |
Ba II | 2 | ... | -0.04+-0.01 | ... | -2.37+-0.01 | -0.04+-0.01 | -0.19+-0.01 | Ba II |
Eu II | 1 | ... | <1.1 | ... | <-1.19 | <1.14 | <-0.67 | Eu II |
Vrad | 90.3 |
Right Ascension : 11 44 22.60 | Declination : -06 26 59.0 | 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 | 100 | 2700 | 91.9 |
2012-03 | N/A | KECKHIRES | 36000 | >150 | 1000 | 90.3 |