HIP44075
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 : 5875 | log g : 4.10 | vturb : 1.10 |
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 | -0.83+-0.03 | ... | ... | -0.74+-0.03 | 0.17+-0.03 | 5.50+-0.03 | Na I |
Mg I | 4 | -0.55+-0.07 | ... | ... | -0.57+-0.07 | 0.34+-0.07 | 7.03+-0.07 | Mg I |
Al I | 3 | -0.57+-0.12 | ... | ... | -0.55+-0.12 | 0.36+-0.12 | 5.90+-0.12 | Al I |
Si I | 15 | -0.63+-0.11 | ... | ... | -0.59+-0.11 | 0.32+-0.11 | 6.92+-0.11 | Si I |
Ca I | 10 | -0.67+-0.08 | ... | ... | -0.65+-0.08 | 0.26+-0.08 | 5.69+-0.08 | Ca I |
Ti I | 9 | -0.65+-0.06 | ... | ... | -0.58+-0.06 | 0.33+-0.06 | 4.37+-0.06 | Ti I |
Ti II | 8 | -0.59+-0.08 | ... | ... | -0.52+-0.08 | 0.39+-0.08 | 4.43+-0.08 | Ti II |
Cr I | 4 | -0.90+-0.17 | ... | ... | -0.87+-0.17 | 0.04+-0.17 | 4.77+-0.17 | Cr I |
Cr II | 5 | -0.90+-0.09 | ... | ... | -0.87+-0.09 | 0.04+-0.09 | 4.77+-0.09 | Cr II |
Fe I | 67 | -0.91+-0.07 | ... | ... | -0.91+-0.07 | ... | 6.59+-0.07 | Fe I |
Fe II | 16 | -0.89+-0.06 | ... | ... | -0.89+-0.06 | ... | 6.61+-0.06 | Fe II |
Ni I | 26 | -0.91+-0.10 | ... | ... | -0.88+-0.10 | 0.03+-0.10 | 5.34+-0.10 | Ni I |
Zn I | 1 | -0.78+-0.00 | ... | ... | -0.74+-0.00 | 0.17+-0.00 | 3.82+-0.00 | Zn I |
Y II | 4 | -0.89+-0.10 | ... | ... | -0.86+-0.10 | 0.05+-0.10 | 1.35+-0.10 | Y II |
Ba II | 4 | -0.81+-0.10 | ... | ... | -0.86+-0.10 | 0.05+-0.10 | 1.32+-0.10 | 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 : 5937+-80 | log g : 4.22+-0.11 | vturb : 1.32+-0.15 |
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 | 2 | ... | 0.03+-0.03 | ... | -0.94+-0.03 | 0.01+-0.03 | 5.30+-0.03 | Na |
Mg | 1 | ... | 0.37+-0.05 | ... | -0.60+-0.05 | 0.35+-0.05 | 7.00+-0.05 | Mg |
Al | 1 | ... | 0.26+-0.04 | ... | -0.72+-0.04 | 0.23+-0.04 | 5.73+-0.04 | Al |
Si | 11 | ... | 0.23+-0.05 | ... | -0.67+-0.05 | 0.28+-0.05 | 6.84+-0.05 | Si |
Ca | 15 | ... | 0.26+-0.05 | ... | -0.67+-0.05 | 0.28+-0.05 | 5.67+-0.05 | Ca |
Ti | 30 | -0.59+-0.09 | 0.31+-0.09 | ... | -0.64+-0.09 | 0.31+-0.09 | 4.31+-0.09 | Ti |
Cr | 15 | ... | -0.01+-0.10 | ... | -0.91+-0.10 | 0.04+-0.10 | 4.73+-0.10 | Cr |
Fe | 158 | -0.90+-0.06 | ... | ... | -0.95+-0.06 | ... | 6.55+-0.06 | Fe |
Fe I | 140 | ... | ... | 6.65 | -0.85 | ... | 6.65 | Fe I |
Fe II | 18 | ... | ... | 6.65 | -0.85 | ... | 6.65 | Fe II |
Ni | 34 | ... | -0.01+-0.07 | ... | -0.90+-0.07 | 0.05+-0.07 | 5.32+-0.07 | Ni |
Zn | 3 | ... | 0.11+-0.08 | ... | -0.75+-0.08 | 0.20+-0.08 | 3.81+-0.08 | Zn |
Y | 6 | ... | 0.09+-0.18 | ... | -0.81+-0.18 | 0.14+-0.18 | 1.40+-0.18 | Y |
Ba | 3 | ... | 0.01+-0.13 | ... | -0.90+-0.13 | 0.05+-0.13 | 1.28+-0.13 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-01-01 | N/A | VLT | 110000 | 300-500 | 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 | ... | 0.08 | ... | -0.74 | 0.17 | 5.50 | Na |
Mg | N/A | ... | 0.39 | ... | -0.54 | 0.37 | 7.06 | Mg |
Ca | N/A | ... | 0.31 | ... | -0.58 | 0.33 | 5.76 | Ca |
Ti | N/A | ... | 0.31 | ... | -0.53 | 0.38 | 4.42 | Ti |
Fe | N/A | -0.91 | ... | ... | -0.91 | ... | 6.59 | Fe |
Ni | N/A | ... | 0.05 | ... | -0.83 | 0.08 | 5.39 | Ni |
Ba | N/A | ... | -0.02 | ... | -0.98 | -0.07 | 1.20 | Ba |