G16-20
taken from 2 paper(s):
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5625 | log g : 3.64 | vturb : 1.5 |
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 | ... | -0.13 | ... | -1.46 | -0.04 | 4.78 | Na |
Mg | N/A | ... | 0.22 | ... | -1.22 | 0.20 | 6.38 | Mg |
Si | N/A | ... | 0.33 | ... | -1.05 | 0.37 | 6.46 | Si |
Ca | N/A | ... | 0.32 | ... | -1.08 | 0.34 | 5.26 | Ca |
Ti | N/A | ... | 0.19 | ... | -1.16 | 0.26 | 3.79 | Ti |
Cr | N/A | ... | -0.07 | ... | -1.46 | -0.04 | 4.18 | Cr |
Fe | N/A | -1.42 | ... | ... | -1.42 | ... | 6.08 | Fe |
Ni | N/A | ... | 0.01 | ... | -1.38 | 0.04 | 4.84 | Ni |
Position
Right Ascension : 15 58 18.62 | Declination : +02 03 06.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-15-0155 | N/A | FIESNOT | 40000 | 185 | N/A | 170.8 |
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
Stellar Parameters
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 |
Mn | N/A | ... | -0.34 | ... | -1.80 | -0.38 | 3.63 | Mn |
Fe | N/A | -1.42 | ... | ... | -1.42 | ... | 6.08 | Fe |
Zn | N/A | ... | 0.09 | ... | -1.29 | 0.13 | 3.27 | Zn |
Y | N/A | ... | -0.13 | ... | -1.52 | -0.10 | 0.69 | Y |
Ba | N/A | ... | -0.22 | ... | -1.69 | -0.27 | 0.49 | Ba |
Position
Right Ascension : 15 58 18.62 | Declination : +02 03 06.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-15-0155 | N/A | FIESNOT | 40000 | 185 | N/A | 170.8 |