HE0508-1555
/J.G.Cohen et al.(2004)/ /J.G.Cohen et al.(2013)/
Abundances In Very Metal-Poor Dwarf Stars
Teff : 6365 | log g : 4.4 | 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 | ... | ... | 5.70+-0.28 | -1.90+-0.28 | 0.53+-0.28 | 5.70+-0.28 | Mg I |
Al I | 2 | ... | ... | 3.91+-0.09 | -2.54+-0.09 | -0.11+-0.09 | 3.91+-0.09 | Al I |
Si I | 1 | ... | ... | 5.23 | -2.28 | 0.15 | 5.23 | Si I |
Ca I | 7 | ... | ... | 4.22+-0.11 | -2.12+-0.11 | 0.31+-0.11 | 4.22+-0.11 | Ca I |
Sc II | 3 | ... | ... | 1.02+-0.03 | -2.13+-0.03 | 0.30+-0.03 | 1.02+-0.03 | Sc II |
Ti I | 5 | ... | ... | 3.23+-0.14 | -1.72+-0.14 | 0.71+-0.14 | 3.23+-0.14 | Ti I |
Ti II | 15 | ... | ... | 3.08+-0.10 | -1.87+-0.10 | 0.56+-0.10 | 3.08+-0.10 | Ti II |
Cr I | 4 | ... | ... | 2.99+-0.04 | -2.65+-0.04 | -0.22+-0.04 | 2.99+-0.04 | Cr I |
Mn I | 2 | ... | ... | 2.35+-0.05 | -3.08+-0.05 | -0.65+-0.05 | 2.35+-0.05 | Mn I |
Fe I | 60 | ... | ... | 5.07+-0.17 | -2.43+-0.17 | ... | 5.07+-0.17 | Fe I |
Fe II | 6 | ... | ... | 5.13+-0.17 | -2.37+-0.17 | ... | 5.13+-0.17 | Fe II |
Co I | 2 | ... | ... | 2.92+-0.11 | -2.07+-0.11 | 0.36+-0.11 | 2.92+-0.11 | Co I |
Ni I | 1 | ... | ... | 3.83 | -2.39 | 0.04 | 3.83 | Ni I |
Sr II | 2 | ... | ... | 0.75+-0.04 | -2.12+-0.04 | 0.31+-0.04 | 0.75+-0.04 | Sr II |
Ba II | 2 | ... | ... | -0.35+-0.01 | -2.53+-0.01 | -0.10+-0.01 | -0.35+-0.01 | Ba II |
Eu II | 1 | ... | ... | <-0.40 | <-0.92 | <1.51 | <-0.40 | Eu II |
Right Ascension : 05 10 35.40 | Declination : -15 51 39.0 | 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 | 100 | 6000 | N/A |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Teff : 6365+-100 | log g : 4.4+-0.25 | vturb : 1.4+-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 | ... | 0.4+-0.22 | ... | -2.09+-0.22 | 0.39+-0.22 | 5.51+-0.22 | Mg I |
Al I | 2 | ... | -0.24+-0.05 | ... | -2.65+-0.05 | -0.17+-0.05 | 3.80+-0.05 | Al I |
Si I | 1 | ... | -0.01 | ... | -2.40 | 0.08 | 5.11 | Si I |
Ca I | 7 | ... | 0.21+-0.09 | ... | -2.20+-0.09 | 0.28+-0.09 | 4.14+-0.09 | Ca I |
Sc II | 3 | ... | 0.31+-0.02 | ... | -2.17+-0.02 | 0.31+-0.02 | 0.98+-0.02 | Sc II |
Ti I | 5 | ... | 0.59+-0.13 | ... | -1.80+-0.13 | 0.68+-0.13 | 3.15+-0.13 | Ti I |
Ti II | 15 | ... | 0.5+-0.11 | ... | -1.89+-0.11 | 0.59+-0.11 | 3.06+-0.11 | Ti II |
Cr I | 4 | ... | -0.3+-0.03 | ... | -2.70+-0.03 | -0.22+-0.03 | 2.94+-0.03 | Cr I |
Mn I | 2 | ... | -0.68+-0.03 | ... | -3.15+-0.03 | -0.67+-0.03 | 2.28+-0.03 | Mn I |
Fe I | N/A | -2.43+-0.12 | ... | ... | -2.48+-0.12 | ... | 5.02+-0.12 | Fe I |
Fe II | 6 | -2.35+-0.16 | 0.08+-0.16 | ... | -2.40+-0.16 | 0.08+-0.16 | 5.10+-0.16 | Fe II |
Co I | 2 | ... | 0.36+-0.09 | ... | -2.14+-0.09 | 0.34+-0.09 | 2.85+-0.09 | Co I |
Ni I | 1 | ... | -0.02 | ... | -2.42 | 0.06 | 3.80 | Ni I |
Sr II | 2 | ... | 0.31+-0.05 | ... | -2.09+-0.05 | 0.39+-0.05 | 0.78+-0.05 | Sr II |
Ba II | 1 | ... | -0.1 | ... | -2.58 | -0.10 | -0.40 | Ba II |
Eu II | 1 | ... | <1.47 | ... | <-0.97 | <1.51 | <-0.45 | Eu II |
Vrad | 88.5 |
Right Ascension : 05 10 35.40 | Declination : -15 51 39.0 | 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 | 80 | 6000 | 88.5 |