HE0105-2202
/J.G.Cohen et al.(2004)/ /J.G.Cohen et al.(2013)/
Abundances In Very Metal-Poor Dwarf Stars
Teff : 6330 | 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 | 4 | ... | ... | 5.47+-0.29 | -2.13+-0.29 | 0.47+-0.29 | 5.47+-0.29 | Mg I |
Al I | 2 | ... | ... | 3.61+-0.05 | -2.84+-0.05 | -0.24+-0.05 | 3.61+-0.05 | Al I |
Si I | 1 | ... | ... | 5.16 | -2.35 | 0.25 | 5.16 | Si I |
Ca I | 4 | ... | ... | 4.02+-0.11 | -2.32+-0.11 | 0.28+-0.11 | 4.02+-0.11 | Ca I |
Sc II | 3 | ... | ... | 0.75+-0.25 | -2.40+-0.25 | 0.20+-0.25 | 0.75+-0.25 | Sc II |
Ti I | 3 | ... | ... | 3.19+-0.16 | -1.76+-0.16 | 0.84+-0.16 | 3.19+-0.16 | Ti I |
Ti II | 11 | ... | ... | 2.75+-0.13 | -2.20+-0.13 | 0.40+-0.13 | 2.75+-0.13 | Ti II |
Cr I | 3 | ... | ... | 2.83+-0.15 | -2.81+-0.15 | -0.21+-0.15 | 2.83+-0.15 | Cr I |
Mn I | 2 | ... | ... | 2.13+-0.08 | -3.30+-0.08 | -0.70+-0.08 | 2.13+-0.08 | Mn I |
Fe I | 53 | ... | ... | 4.90+-0.18 | -2.60+-0.18 | ... | 4.90+-0.18 | Fe I |
Fe II | 4 | ... | ... | 4.92+-0.17 | -2.58+-0.17 | ... | 4.92+-0.17 | Fe II |
Co I | 2 | ... | ... | 2.86+-0.03 | -2.13+-0.03 | 0.47+-0.03 | 2.86+-0.03 | Co I |
Ni I | 1 | ... | ... | 3.48 | -2.74 | -0.14 | 3.48 | Ni I |
Sr II | 2 | ... | ... | -0.02+-0.04 | -2.89+-0.04 | -0.29+-0.04 | -0.02+-0.04 | Sr II |
Ba II | 2 | ... | ... | -0.79+-0.20 | -2.97+-0.20 | -0.37+-0.20 | -0.79+-0.20 | Ba II |
Eu II | 1 | ... | ... | <-0.37 | <-0.89 | <1.71 | <-0.37 | Eu II |
Right Ascension : 01 07 31.20 | Declination : -21 46 06.0 | 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 | 65 | 3600 | N/A |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Teff : 6330+-100 | log g : 4.4+-0.25 | vturb : 1.6+-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 | ... | 0.42+-0.23 | ... | -2.19+-0.23 | 0.41+-0.23 | 5.41+-0.23 | Mg I |
Al I | 2 | ... | -0.32+-0.05 | ... | -2.85+-0.05 | -0.25+-0.05 | 3.60+-0.05 | Al I |
Si I | 1 | ... | 0.11 | ... | -2.40 | 0.20 | 5.11 | Si I |
Ca I | 4 | ... | 0.2+-0.11 | ... | -2.33+-0.11 | 0.27+-0.11 | 4.01+-0.11 | Ca I |
Sc II | 3 | ... | 0.2+-0.25 | ... | -2.40+-0.25 | 0.20+-0.25 | 0.75+-0.25 | Sc II |
Ti I | 3 | ... | 0.74+-0.16 | ... | -1.77+-0.16 | 0.83+-0.16 | 3.18+-0.16 | Ti I |
Ti II | 11 | ... | 0.31+-0.13 | ... | -2.20+-0.13 | 0.40+-0.13 | 2.75+-0.13 | Ti II |
Cr I | 3 | ... | -0.29+-0.15 | ... | -2.81+-0.15 | -0.21+-0.15 | 2.83+-0.15 | Cr I |
Mn I | 2 | ... | -0.71+-0.08 | ... | -3.30+-0.08 | -0.70+-0.08 | 2.13+-0.08 | Mn I |
Fe I | N/A | -2.55+-0.15 | ... | ... | -2.60+-0.15 | ... | 4.90+-0.15 | Fe I |
Fe II | 4 | -2.53+-0.17 | 0.02+-0.17 | ... | -2.58+-0.17 | 0.02+-0.17 | 4.92+-0.17 | Fe II |
Co I | 2 | ... | 0.49+-0.03 | ... | -2.13+-0.03 | 0.47+-0.03 | 2.86+-0.03 | Co I |
Ni I | 1 | ... | -0.22 | ... | -2.74 | -0.14 | 3.48 | Ni I |
Sr II | 2 | ... | -0.38+-0.04 | ... | -2.90+-0.04 | -0.30+-0.04 | -0.03+-0.04 | Sr II |
Ba II | 1 | ... | -0.51 | ... | -3.11 | -0.51 | -0.93 | Ba II |
Eu II | 1 | ... | <1.66 | ... | <-0.90 | <1.70 | <-0.38 | Eu II |
Vrad | -77.3 |
Right Ascension : 01 07 31.20 | Declination : -21 46 06.0 | 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 | 55 | 3600 | -77.3 |