G96-20
taken from 3 paper(s):
/H.L.Yan et al.(2016)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
| Teff : 6293 | log g : 4.41 | 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 |
|---|
| Fe | N/A | -0.89 | ... | ... | -0.89 | ... | 6.61 | Fe |
| Cu | N/A | ... | -0.09+-0.01 | ... | -0.96+-0.01 | -0.07+-0.01 | 3.23+-0.01 | Cu |
Position
| Right Ascension : 05 05 28.71 | Declination : +40 15 26.4 | 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 | FIESNOT | 40000 | 140-200 | N/A | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
| Teff : 6293 | log g : 4.41 | 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 | ... | -0.67 | 0.22 | 5.57 | Na |
| Mg | N/A | ... | 0.3 | ... | -0.61 | 0.28 | 6.99 | Mg |
| Si | N/A | ... | 0.3 | ... | -0.55 | 0.34 | 6.96 | Si |
| Ca | N/A | ... | 0.27 | ... | -0.60 | 0.29 | 5.74 | Ca |
| Ti | N/A | ... | 0.25 | ... | -0.57 | 0.32 | 4.38 | Ti |
| Cr | N/A | ... | -0.06 | ... | -0.92 | -0.03 | 4.72 | Cr |
| Fe | N/A | -0.89 | ... | ... | -0.89 | ... | 6.61 | Fe |
Position
| Right Ascension : 05 05 28.71 | Declination : +40 15 26.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-12-01-0039 | N/A | FIESNOT | 40000 | 180 | N/A | 105.7 |
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 | ... | -0.28 | ... | -1.21 | -0.32 | 4.22 | Mn |
| Fe | N/A | -0.89 | ... | ... | -0.89 | ... | 6.61 | Fe |
| Cu | N/A | ... | -0.13 | ... | -1.00 | -0.11 | 3.19 | Cu |
| Zn | N/A | ... | 0.11 | ... | -0.74 | 0.15 | 3.82 | Zn |
| Y | N/A | ... | 0.28 | ... | -0.58 | 0.31 | 1.63 | Y |
| Ba | N/A | ... | 0.68 | ... | -0.26 | 0.63 | 1.92 | Ba |
Position
| Right Ascension : 05 05 28.71 | Declination : +40 15 26.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-12-01-0039 | N/A | FIESNOT | 40000 | 180 | N/A | 105.7 |