HIP12611
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 | 0.38+-0.03 | ... | ... | 0.47+-0.03 | 0.21+-0.03 | 6.71+-0.03 | Na I |
Mg I | 6 | 0.28+-0.05 | ... | ... | 0.26+-0.05 | 0.00+-0.05 | 7.86+-0.05 | Mg I |
Al I | 6 | 0.41+-0.05 | ... | ... | 0.43+-0.05 | 0.17+-0.05 | 6.88+-0.05 | Al I |
Si I | 31 | 0.37+-0.10 | ... | ... | 0.41+-0.10 | 0.15+-0.10 | 7.92+-0.10 | Si I |
Ca I | 22 | 0.30+-0.16 | ... | ... | 0.32+-0.16 | 0.06+-0.16 | 6.66+-0.16 | Ca I |
Ti I | 31 | 0.29+-0.24 | ... | ... | 0.36+-0.24 | 0.10+-0.24 | 5.31+-0.24 | Ti I |
Ti II | 18 | 0.31+-0.26 | ... | ... | 0.38+-0.26 | 0.12+-0.26 | 5.33+-0.26 | Ti II |
Cr I | 14 | 0.28+-0.15 | ... | ... | 0.31+-0.15 | 0.05+-0.15 | 5.95+-0.15 | Cr I |
Cr II | 9 | 0.25+-0.17 | ... | ... | 0.28+-0.17 | 0.02+-0.17 | 5.92+-0.17 | Cr II |
Fe I | 149 | 0.26+-0.12 | ... | ... | 0.26+-0.12 | ... | 7.76+-0.12 | Fe I |
Fe II | 24 | 0.28+-0.12 | ... | ... | 0.28+-0.12 | ... | 7.78+-0.12 | Fe II |
Ni I | 53 | 0.33+-0.14 | ... | ... | 0.36+-0.14 | 0.10+-0.14 | 6.58+-0.14 | Ni I |
Zn I | 2 | 0.34+-0.18 | ... | ... | 0.38+-0.18 | 0.12+-0.18 | 4.94+-0.18 | Zn I |
Y II | 7 | 0.25+-0.32 | ... | ... | 0.28+-0.32 | 0.02+-0.32 | 2.49+-0.32 | Y II |
Ba II | 4 | 0.17+-0.07 | ... | ... | 0.12+-0.07 | -0.14+-0.07 | 2.30+-0.07 | Ba II |
Position
Right Ascension : 02 42 08.40 | Declination : -46 31 28.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
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 : 5431+-108 | log g : 3.97+-0.15 | vturb : 1.37+-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 |
O | 3 | ... | -0.27+-0.30 | ... | 0.06+-0.30 | -0.25+-0.30 | 8.75+-0.30 | O |
Na | 4 | ... | 0.08+-0.12 | ... | 0.37+-0.12 | 0.06+-0.12 | 6.61+-0.12 | Na |
Mg | 6 | ... | -0.08+-0.12 | ... | 0.21+-0.12 | -0.10+-0.12 | 7.81+-0.12 | Mg |
Al | 7 | ... | 0.08+-0.13 | ... | 0.36+-0.13 | 0.05+-0.13 | 6.81+-0.13 | Al |
Si | 31 | ... | 0.00+-0.14 | ... | 0.36+-0.14 | 0.05+-0.14 | 7.87+-0.14 | Si |
Ca | 23 | ... | -0.02+-0.09 | ... | 0.31+-0.09 | -0.00+-0.09 | 6.65+-0.09 | Ca |
Ti | 41 | 0.43+-0.18 | 0.07+-0.18 | ... | 0.38+-0.18 | 0.07+-0.18 | 5.33+-0.18 | Ti |
Cr | 21 | ... | -0.02+-0.09 | ... | 0.34+-0.09 | 0.03+-0.09 | 5.98+-0.09 | Cr |
Fe | 106 | 0.36+-0.18 | ... | ... | 0.31+-0.18 | ... | 7.81+-0.18 | Fe |
Fe I | 78 | ... | ... | 7.92 | 0.42 | ... | 7.92 | Fe I |
Fe II | 28 | ... | ... | 7.93 | 0.43 | ... | 7.93 | Fe II |
Ni | 45 | ... | 0.04+-0.10 | ... | 0.41+-0.10 | 0.10+-0.10 | 6.63+-0.10 | Ni |
Zn | 3 | ... | 0.13+-0.15 | ... | 0.53+-0.15 | 0.22+-0.15 | 5.09+-0.15 | Zn |
Y | 6 | ... | 0.02+-0.19 | ... | 0.38+-0.19 | 0.07+-0.19 | 2.59+-0.19 | Y |
Ba | 4 | ... | -0.10+-0.14 | ... | 0.25+-0.14 | -0.06+-0.14 | 2.43+-0.14 | Ba |
Position
Right Ascension : 02 42 08.40 | Declination : -46 31 28.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-09-01 | N/A | FEROSESO | 48000 | 150 | N/A | N/A |
Stellar Chemical Signatures and Hierarchical Galaxy Formation
Position
Right Ascension : 02 42 08.40 | Declination : -46 31 28.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log