HIP12306
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
Stellar Parameters
Teff : 5765 | log g : 4.20 | vturb : 0.90 |
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 | -0.47+-0.03 | ... | ... | -0.38+-0.03 | 0.15+-0.03 | 5.86+-0.03 | Na I |
Mg I | 3 | -0.23+-0.07 | ... | ... | -0.25+-0.07 | 0.28+-0.07 | 7.35+-0.07 | Mg I |
Al I | 4 | -0.30+-0.05 | ... | ... | -0.28+-0.05 | 0.25+-0.05 | 6.17+-0.05 | Al I |
Si I | 17 | -0.38+-0.07 | ... | ... | -0.34+-0.07 | 0.19+-0.07 | 7.17+-0.07 | Si I |
Ca I | 8 | -0.37+-0.08 | ... | ... | -0.35+-0.08 | 0.18+-0.08 | 5.99+-0.08 | Ca I |
Ti I | 8 | -0.37+-0.06 | ... | ... | -0.30+-0.06 | 0.23+-0.06 | 4.65+-0.06 | Ti I |
Ti II | 9 | -0.42+-0.12 | ... | ... | -0.35+-0.12 | 0.18+-0.12 | 4.60+-0.12 | Ti II |
Cr I | 6 | -0.55+-0.03 | ... | ... | -0.52+-0.03 | 0.01+-0.03 | 5.12+-0.03 | Cr I |
Cr II | 5 | -0.56+-0.06 | ... | ... | -0.53+-0.06 | 0.00+-0.06 | 5.11+-0.06 | Cr II |
Fe I | 80 | -0.53+-0.07 | ... | ... | -0.53+-0.07 | ... | 6.97+-0.07 | Fe I |
Fe II | 19 | -0.58+-0.07 | ... | ... | -0.58+-0.07 | ... | 6.92+-0.07 | Fe II |
Ni I | 33 | -0.53+-0.05 | ... | ... | -0.50+-0.05 | 0.03+-0.05 | 5.72+-0.05 | Ni I |
Zn I | 1 | -0.46+-0.00 | ... | ... | -0.42+-0.00 | 0.11+-0.00 | 4.14+-0.00 | Zn I |
Y II | 4 | -0.74+-0.08 | ... | ... | -0.71+-0.08 | -0.18+-0.08 | 1.50+-0.08 | Y II |
Ba II | 4 | -0.62+-0.05 | ... | ... | -0.67+-0.05 | -0.14+-0.05 | 1.51+-0.05 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-11-01 | N/A | NOTSOFIN | 80000 | >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 : 5832+-85 | log g : 4.44+-0.13 | vturb : 0.95+-0.12 |
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 | 4 | ... | 0.06+-0.04 | ... | -0.53+-0.04 | 0.04+-0.04 | 5.71+-0.04 | Na |
Mg | 3 | ... | 0.28+-0.08 | ... | -0.31+-0.08 | 0.26+-0.08 | 7.29+-0.08 | Mg |
Al | 5 | ... | 0.19+-0.06 | ... | -0.41+-0.06 | 0.16+-0.06 | 6.04+-0.06 | Al |
Si | 17 | ... | 0.15+-0.06 | ... | -0.37+-0.06 | 0.20+-0.06 | 7.14+-0.06 | Si |
Ca | 12 | ... | 0.13+-0.06 | ... | -0.42+-0.06 | 0.15+-0.06 | 5.92+-0.06 | Ca |
Ti | 25 | -0.28+-0.08 | 0.24+-0.08 | ... | -0.33+-0.08 | 0.24+-0.08 | 4.62+-0.08 | Ti |
Cr | 11 | ... | 0.02+-0.08 | ... | -0.50+-0.08 | 0.07+-0.08 | 5.14+-0.08 | Cr |
Fe | 105 | -0.52+-0.08 | ... | ... | -0.57+-0.08 | ... | 6.93+-0.08 | Fe |
Fe I | 81 | ... | ... | 7.05 | -0.45 | ... | 7.05 | Fe I |
Fe II | 24 | ... | ... | 7.05 | -0.45 | ... | 7.05 | Fe II |
Ni | 34 | ... | 0.05+-0.07 | ... | -0.46+-0.07 | 0.11+-0.07 | 5.76+-0.07 | Ni |
Zn | 1 | ... | 0.07+-0.06 | ... | -0.41+-0.06 | 0.16+-0.06 | 4.15+-0.06 | Zn |
Y | 5 | ... | -0.11+-0.17 | ... | -0.63+-0.17 | -0.06+-0.17 | 1.58+-0.17 | Y |
Ba | 4 | ... | -0.03+-0.09 | ... | -0.56+-0.09 | 0.01+-0.09 | 1.62+-0.09 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-01-01 | N/A | NOTSOFIN | 80000 | 250 | 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 | ... | 0.1 | ... | -0.44 | 0.19 | 5.80 | Na |
Mg | N/A | ... | 0.31 | ... | -0.34 | 0.29 | 7.26 | Mg |
Ca | N/A | ... | 0.17 | ... | -0.44 | 0.19 | 5.90 | Ca |
Ti | N/A | ... | 0.19 | ... | -0.37 | 0.26 | 4.58 | Ti |
Fe | N/A | -0.63 | ... | ... | -0.63 | ... | 6.87 | Fe |
Ni | N/A | ... | 0.07 | ... | -0.53 | 0.10 | 5.69 | Ni |
Y | N/A | ... | -0.23 | ... | -0.83 | -0.20 | 1.38 | Y |
Ba | N/A | ... | -0.07 | ... | -0.75 | -0.12 | 1.43 | Ba |
Eu | N/A | ... | 0.11 | ... | -0.53 | 0.10 | -0.01 | Eu |