CD-51_4628
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 : 6153 | log g : 4.31 | vturb : 1.4 |
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 | ... | -0.26 | ... | -1.47 | -0.17 | 4.77 | Na |
Mg | N/A | ... | 0.13 | ... | -1.19 | 0.11 | 6.41 | Mg |
Si | N/A | ... | 0.19 | ... | -1.07 | 0.23 | 6.44 | Si |
Ca | N/A | ... | 0.31 | ... | -0.97 | 0.33 | 5.37 | Ca |
Ti | N/A | ... | 0.24 | ... | -0.99 | 0.31 | 3.96 | Ti |
Cr | N/A | ... | 0.00 | ... | -1.27 | 0.03 | 4.37 | Cr |
Fe | N/A | -1.30 | ... | ... | -1.30 | ... | 6.20 | Fe |
Ni | N/A | ... | -0.1 | ... | -1.37 | -0.07 | 4.85 | Ni |
Position
Right Ascension : 10 17 14.88 | Declination : -52 29 18.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-18-0615 | N/A | VLT | 55000 | 280 | N/A | 197.9 |
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 | ... | -0.36 | ... | -1.70 | -0.40 | 3.73 | Mn |
Fe | N/A | -1.30 | ... | ... | -1.30 | ... | 6.20 | Fe |
Zn | N/A | ... | 0.00 | ... | -1.26 | 0.04 | 3.30 | Zn |
Y | N/A | ... | -0.11 | ... | -1.38 | -0.08 | 0.83 | Y |
Ba | N/A | ... | -0.16 | ... | -1.51 | -0.21 | 0.67 | Ba |
Position
Right Ascension : 10 17 14.88 | Declination : -52 29 18.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-18-0615 | N/A | VLT | 55000 | 280 | N/A | 197.9 |