HIP17147
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 | -0.75+-0.04 | ... | ... | -0.66+-0.04 | 0.18+-0.04 | 5.58+-0.04 | Na I |
Mg I | 6 | -0.44+-0.04 | ... | ... | -0.46+-0.04 | 0.38+-0.04 | 7.14+-0.04 | Mg I |
Al I | 4 | -0.50+-0.01 | ... | ... | -0.48+-0.01 | 0.36+-0.01 | 5.97+-0.01 | Al I |
Si I | 29 | -0.57+-0.10 | ... | ... | -0.53+-0.10 | 0.31+-0.10 | 6.98+-0.10 | Si I |
Ca I | 22 | -0.58+-0.12 | ... | ... | -0.56+-0.12 | 0.28+-0.12 | 5.78+-0.12 | Ca I |
Ti I | 25 | -0.53+-0.10 | ... | ... | -0.46+-0.10 | 0.38+-0.10 | 4.49+-0.10 | Ti I |
Ti II | 18 | -0.55+-0.12 | ... | ... | -0.48+-0.12 | 0.36+-0.12 | 4.47+-0.12 | Ti II |
Cr I | 10 | -0.75+-0.13 | ... | ... | -0.72+-0.13 | 0.12+-0.13 | 4.92+-0.13 | Cr I |
Cr II | 7 | -0.92+-0.07 | ... | ... | -0.89+-0.07 | -0.05+-0.07 | 4.75+-0.07 | Cr II |
Fe I | 120 | -0.84+-0.09 | ... | ... | -0.84+-0.09 | ... | 6.66+-0.09 | Fe I |
Fe II | 24 | -0.88+-0.12 | ... | ... | -0.88+-0.12 | ... | 6.62+-0.12 | Fe II |
Ni I | 42 | -0.83+-0.14 | ... | ... | -0.80+-0.14 | 0.04+-0.14 | 5.42+-0.14 | Ni I |
Zn I | 2 | -0.72+-0.04 | ... | ... | -0.68+-0.04 | 0.16+-0.04 | 3.88+-0.04 | Zn I |
Y II | 6 | -0.88+-0.16 | ... | ... | -0.85+-0.16 | -0.01+-0.16 | 1.36+-0.16 | Y II |
Ba II | 4 | -0.81+-0.06 | ... | ... | -0.86+-0.06 | -0.02+-0.06 | 1.32+-0.06 | 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 : 5970+-150 | log g : 4.52+-0.15 | vturb : 1.27+-1.00 |
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 | ... | 0.53 | ... | -0.31 | 0.55 | 8.38 | O |
Na | 4 | ... | 0.06 | ... | -0.82 | 0.04 | 5.42 | Na |
Mg | 6 | ... | 0.35 | ... | -0.53 | 0.33 | 7.07 | Mg |
Al | 4 | ... | 0.33 | ... | -0.56 | 0.30 | 5.89 | Al |
Si | 29 | ... | 0.23 | ... | -0.58 | 0.28 | 6.93 | Si |
Ca | 22 | ... | 0.24 | ... | -0.60 | 0.26 | 5.74 | Ca |
Ti | 43 | -0.48 | 0.33 | ... | -0.53 | 0.33 | 4.42 | Ti |
Cr | 17 | ... | 0.03 | ... | -0.78 | 0.08 | 4.86 | Cr |
Fe | 150 | -0.81+-0.15 | ... | ... | -0.86+-0.15 | ... | 6.64+-0.15 | Fe |
Fe I | 121 | ... | ... | 6.75 | -0.75 | ... | 6.75 | Fe I |
Fe II | 29 | ... | ... | 6.75 | -0.75 | ... | 6.75 | Fe II |
Ni | 43 | ... | 0.01 | ... | -0.79 | 0.07 | 5.43 | Ni |
Zn | 3 | ... | 0.09 | ... | -0.68 | 0.18 | 3.88 | Zn |
Y | 6 | ... | 0.12 | ... | -0.69 | 0.17 | 1.52 | Y |
Ba | 4 | ... | -0.01 | ... | -0.83 | 0.03 | 1.35 | 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 | ... | 0.09 | ... | -0.66 | 0.18 | 5.58 | Na |
Mg | N/A | ... | 0.4 | ... | -0.46 | 0.38 | 7.14 | Mg |
Ca | N/A | ... | 0.26 | ... | -0.56 | 0.28 | 5.78 | Ca |
Ti | N/A | ... | 0.3 | ... | -0.47 | 0.37 | 4.48 | Ti |
Fe | N/A | -0.84 | ... | ... | -0.84 | ... | 6.66 | Fe |
Ni | N/A | ... | 0.01 | ... | -0.80 | 0.04 | 5.42 | Ni |
Y | N/A | ... | 0.05 | ... | -0.76 | 0.08 | 1.45 | Y |
Ba | N/A | ... | 0.11 | ... | -0.78 | 0.06 | 1.40 | Ba |