HD88446
HIP49988 in T.Bensby+,AAP, 562, A71, 2014
taken from 3 paper(s):
/T.Gehren et al.(2006)/
/T.Bensby et al.(2014)/
/K.A.Venn et al.(2004)/

Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 5915 | log g : 4.03+-0.11 | vturb : 1.6 |
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 | 6 | ... | -0.00 | ... | -0.35 | 0.08 | 5.89 | Na I |
Mg I | 7 | ... | 0.02 | ... | -0.44 | -0.01 | 7.16 | Mg I |
Al I | 5 | ... | -0.08 | ... | -0.50 | -0.07 | 5.95 | Al I |
Fe | N/A | -0.44 | ... | ... | -0.43 | ... | 7.07 | Fe |
Position
Right Ascension : 10 12 19.08 | Declination : +17 17 57.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 200 | 4200 | 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 : 6003+-46 | log g : 4.02+-0.07 | vturb : 1.16+-0.07 |
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 | ... | 0.15+-0.10 | ... | -0.31+-0.10 | 0.17+-0.10 | 8.38+-0.10 | O |
Na | 4 | ... | 0.00+-0.04 | ... | -0.50+-0.04 | -0.02+-0.04 | 5.74+-0.04 | Na |
Mg | 4 | ... | 0.16+-0.04 | ... | -0.34+-0.04 | 0.14+-0.04 | 7.26+-0.04 | Mg |
Al | 7 | ... | 0.06+-0.04 | ... | -0.45+-0.04 | 0.03+-0.04 | 6.00+-0.04 | Al |
Si | 25 | ... | 0.03+-0.03 | ... | -0.40+-0.03 | 0.08+-0.03 | 7.11+-0.03 | Si |
Ca | 18 | ... | 0.08+-0.12 | ... | -0.38+-0.12 | 0.10+-0.12 | 5.96+-0.12 | Ca |
Ti | 26 | -0.37+-0.05 | 0.06+-0.05 | ... | -0.42+-0.05 | 0.06+-0.05 | 4.53+-0.05 | Ti |
Cr | 13 | ... | -0.02+-0.06 | ... | -0.45+-0.06 | 0.03+-0.06 | 5.19+-0.06 | Cr |
Fe | 206 | -0.43+-0.04 | ... | ... | -0.48+-0.04 | ... | 7.02+-0.04 | Fe |
Fe I | 182 | ... | ... | 7.14 | -0.36 | ... | 7.14 | Fe I |
Fe II | 24 | ... | ... | 7.14 | -0.36 | ... | 7.14 | Fe II |
Ni | 44 | ... | -0.06+-0.04 | ... | -0.48+-0.04 | -0.00+-0.04 | 5.74+-0.04 | Ni |
Zn | 3 | ... | 0.00+-0.04 | ... | -0.39+-0.04 | 0.09+-0.04 | 4.17+-0.04 | Zn |
Y | 6 | ... | 0.53+-0.10 | ... | 0.10+-0.10 | 0.58+-0.10 | 2.31+-0.10 | Y |
Ba | 3 | ... | 0.76+-0.06 | ... | 0.32+-0.06 | 0.80+-0.06 | 2.50+-0.06 | Ba |
Position
Right Ascension : 10 12 19.08 | Declination : +17 17 57.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-04-01 | N/A | MIKELCO | 65000 | 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 | ... | 0.06 | ... | -0.20 | 0.15 | 6.04 | Na |
Mg | N/A | ... | 0.15 | ... | -0.22 | 0.13 | 7.38 | Mg |
Ca | N/A | ... | 0.07 | ... | -0.26 | 0.09 | 6.08 | Ca |
Ti | N/A | ... | 0.1 | ... | -0.18 | 0.17 | 4.77 | Ti |
Fe | N/A | -0.35 | ... | ... | -0.35 | ... | 7.15 | Fe |
Ni | N/A | ... | -0.01 | ... | -0.33 | 0.02 | 5.89 | Ni |
Y | N/A | ... | 0.58 | ... | 0.26 | 0.61 | 2.47 | Y |
Ba | N/A | ... | 0.66 | ... | 0.26 | 0.61 | 2.44 | Ba |
Eu | N/A | ... | 0.24 | ... | -0.12 | 0.23 | 0.40 | Eu |
Position
Right Ascension : 10 12 19.08 | Declination : +17 17 57.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log