G63-26
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 : 6043 | log g : 4.18 | vturb : 1.8 |
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 | ... | -1.55 | 0.01 | 4.69 | Na |
Mg | N/A | ... | 0.35 | ... | -1.23 | 0.33 | 6.37 | Mg |
Si | N/A | ... | 0.49 | ... | -1.03 | 0.53 | 6.48 | Si |
Ca | N/A | ... | 0.37 | ... | -1.17 | 0.39 | 5.17 | Ca |
Ti | N/A | ... | 0.28 | ... | -1.21 | 0.35 | 3.74 | Ti |
Cr | N/A | ... | -0.01 | ... | -1.54 | 0.02 | 4.10 | Cr |
Fe | N/A | -1.56 | ... | ... | -1.56 | ... | 5.94 | Fe |
Ni | N/A | ... | 0.06 | ... | -1.47 | 0.09 | 4.75 | Ni |
Position
Right Ascension : 13 24 30.60 | Declination : +20 27 22.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-03-23-0652 | N/A | VLT | 55000 | 240 | N/A | 57.4 |
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 | ... | -0.32 | ... | -1.92 | -0.36 | 3.51 | Mn |
Fe | N/A | -1.56 | ... | ... | -1.56 | ... | 5.94 | Fe |
Zn | N/A | ... | 0.16 | ... | -1.36 | 0.20 | 3.20 | Zn |
Y | N/A | ... | 0.17 | ... | -1.36 | 0.20 | 0.85 | Y |
Ba | N/A | ... | 0.11 | ... | -1.50 | 0.06 | 0.68 | Ba |
Position
Right Ascension : 13 24 30.60 | Declination : +20 27 22.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-03-23-0652 | N/A | VLT | 55000 | 240 | N/A | 57.4 |