G119-64
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 : 6181 | log g : 4.18 | 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 | ... | -0.15 | ... | -1.54 | -0.06 | 4.70 | Na |
Mg | N/A | ... | 0.25 | ... | -1.25 | 0.23 | 6.35 | Mg |
Si | N/A | ... | 0.21 | ... | -1.23 | 0.25 | 6.28 | Si |
Ca | N/A | ... | 0.37 | ... | -1.09 | 0.39 | 5.25 | Ca |
Ti | N/A | ... | 0.29 | ... | -1.12 | 0.36 | 3.83 | Ti |
Cr | N/A | ... | -0.01 | ... | -1.46 | 0.02 | 4.18 | Cr |
Fe | N/A | -1.48 | ... | ... | -1.48 | ... | 6.02 | Fe |
Ni | N/A | ... | -0.06 | ... | -1.51 | -0.03 | 4.71 | Ni |
Position
Right Ascension : 11 12 48.00 | Declination : +35 43 43.9 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-17-2108 | N/A | FIESNOT | 40000 | 210 | N/A | -195.6 |
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 | ... | -1.86 | -0.38 | 3.57 | Mn |
Fe | N/A | -1.48 | ... | ... | -1.48 | ... | 6.02 | Fe |
Zn | N/A | ... | 0.02 | ... | -1.42 | 0.06 | 3.14 | Zn |
Y | N/A | ... | -0.08 | ... | -1.53 | -0.05 | 0.68 | Y |
Ba | N/A | ... | -0.23 | ... | -1.76 | -0.28 | 0.42 | Ba |
Position
Right Ascension : 11 12 48.00 | Declination : +35 43 43.9 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-17-2108 | N/A | FIESNOT | 40000 | 210 | N/A | -195.6 |