HIP85007
taken from 3 paper(s):
/T.Bensby et al.(2005)/
/T.Bensby et al.(2014)/
/K.A.Venn et al.(2004)/
alpha-, r-, and s-process element trends in the Galactic thin and thick disks
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na I | 4 | -0.33+-0.06 | ... | ... | -0.24+-0.06 | 0.15+-0.06 | 6.00+-0.06 | Na I |
Mg I | 6 | -0.34+-0.04 | ... | ... | -0.36+-0.04 | 0.03+-0.04 | 7.24+-0.04 | Mg I |
Al I | 6 | -0.38+-0.04 | ... | ... | -0.36+-0.04 | 0.03+-0.04 | 6.09+-0.04 | Al I |
Si I | 32 | -0.37+-0.07 | ... | ... | -0.33+-0.07 | 0.06+-0.07 | 7.18+-0.07 | Si I |
Ca I | 22 | -0.37+-0.08 | ... | ... | -0.35+-0.08 | 0.04+-0.08 | 5.99+-0.08 | Ca I |
Ti I | 23 | -0.39+-0.10 | ... | ... | -0.32+-0.10 | 0.07+-0.10 | 4.63+-0.10 | Ti I |
Ti II | 18 | -0.37+-0.12 | ... | ... | -0.30+-0.12 | 0.09+-0.12 | 4.65+-0.12 | Ti II |
Cr I | 11 | -0.45+-0.07 | ... | ... | -0.42+-0.07 | -0.03+-0.07 | 5.22+-0.07 | Cr I |
Cr II | 9 | -0.44+-0.06 | ... | ... | -0.41+-0.06 | -0.02+-0.06 | 5.23+-0.06 | Cr II |
Fe I | 132 | -0.39+-0.09 | ... | ... | -0.39+-0.09 | ... | 7.11+-0.09 | Fe I |
Fe II | 23 | -0.39+-0.06 | ... | ... | -0.39+-0.06 | ... | 7.11+-0.06 | Fe II |
Ni I | 50 | -0.45+-0.08 | ... | ... | -0.42+-0.08 | -0.03+-0.08 | 5.80+-0.08 | Ni I |
Zn I | 2 | -0.34+-0.09 | ... | ... | -0.30+-0.09 | 0.09+-0.09 | 4.26+-0.09 | Zn I |
Y II | 7 | -0.54+-0.18 | ... | ... | -0.51+-0.18 | -0.12+-0.18 | 1.70+-0.18 | Y II |
Ba II | 4 | -0.24+-0.01 | ... | ... | -0.29+-0.01 | 0.10+-0.01 | 1.89+-0.01 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-09-01 | N/A | FEROSESO | 48000 | 150-250 | N/A | N/A |
Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the solar neighbourhood
Stellar Parameters
Teff : 6064+-128 | log g : 4.32+-0.19 | vturb : 1.30+-0.11 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
O | 3 | ... | 0.06+-0.25 | ... | -0.36+-0.25 | 0.08+-0.25 | 8.33+-0.25 | O |
Na | 4 | ... | 0.05+-0.05 | ... | -0.41+-0.05 | 0.03+-0.05 | 5.83+-0.05 | Na |
Mg | 6 | ... | 0.07+-0.07 | ... | -0.39+-0.07 | 0.05+-0.07 | 7.21+-0.07 | Mg |
Al | 6 | ... | 0.01+-0.06 | ... | -0.46+-0.06 | -0.02+-0.06 | 5.99+-0.06 | Al |
Si | 32 | ... | 0.00+-0.07 | ... | -0.39+-0.07 | 0.05+-0.07 | 7.12+-0.07 | Si |
Ca | 22 | ... | 0.03+-0.07 | ... | -0.39+-0.07 | 0.05+-0.07 | 5.95+-0.07 | Ca |
Ti | 40 | -0.39+-0.11 | 0.00+-0.11 | ... | -0.44+-0.11 | -0.00+-0.11 | 4.51+-0.11 | Ti |
Cr | 20 | ... | -0.06+-0.12 | ... | -0.45+-0.12 | -0.01+-0.12 | 5.19+-0.12 | Cr |
Fe | 161 | -0.39+-0.10 | ... | ... | -0.44+-0.10 | ... | 7.06+-0.10 | Fe |
Fe I | 132 | ... | ... | 7.17 | -0.33 | ... | 7.17 | Fe I |
Fe II | 29 | ... | ... | 7.17 | -0.33 | ... | 7.17 | Fe II |
Ni | 51 | ... | -0.04+-0.10 | ... | -0.42+-0.10 | 0.02+-0.10 | 5.80+-0.10 | Ni |
Zn | 3 | ... | -0.06+-0.14 | ... | -0.41+-0.14 | 0.03+-0.14 | 4.15+-0.14 | Zn |
Y | 7 | ... | -0.17+-0.25 | ... | -0.56+-0.25 | -0.12+-0.25 | 1.65+-0.25 | Y |
Ba | 4 | ... | -0.02+-0.11 | ... | -0.42+-0.11 | 0.02+-0.11 | 1.76+-0.11 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-01-01 | N/A | FEROSESO | 48000 | 150 | N/A | N/A |
Stellar Chemical Signatures and Hierarchical Galaxy Formation
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na | N/A | ... | 0.06 | ... | -0.24 | 0.15 | 6.00 | Na |
Mg | N/A | ... | 0.05 | ... | -0.36 | 0.03 | 7.24 | Mg |
Ca | N/A | ... | 0.02 | ... | -0.35 | 0.04 | 5.99 | Ca |
Ti | N/A | ... | 0.01 | ... | -0.31 | 0.08 | 4.64 | Ti |
Fe | N/A | -0.39 | ... | ... | -0.39 | ... | 7.11 | Fe |
Ni | N/A | ... | -0.06 | ... | -0.42 | -0.03 | 5.80 | Ni |
Y | N/A | ... | -0.14 | ... | -0.50 | -0.11 | 1.71 | Y |
Ba | N/A | ... | 0.11 | ... | -0.33 | 0.06 | 1.85 | Ba |
Eu | N/A | ... | -0.04 | ... | -0.44 | -0.05 | 0.08 | Eu |