CD-43_6810
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 : 5945 | log g : 4.26 | vturb : 1.3 |
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 | -0.43 | ... | ... | -0.43 | ... | 7.07 | Fe |
| Cu | N/A | ... | -0.07+-0.01 | ... | -0.48+-0.01 | -0.05+-0.01 | 3.71+-0.01 | Cu |
Position
| Right Ascension : 11 08 40.07 | Declination : -44 15 33.7 | 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 | VLT | 55000 | 250-500 | N/A | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
| Teff : 5945 | log g : 4.26 | vturb : 1.3 |
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 | ... | -0.19 | 0.24 | 6.05 | Na |
| Mg | N/A | ... | 0.28 | ... | -0.17 | 0.26 | 7.43 | Mg |
| Si | N/A | ... | 0.23 | ... | -0.16 | 0.27 | 7.35 | Si |
| Ca | N/A | ... | 0.21 | ... | -0.20 | 0.23 | 6.14 | Ca |
| Ti | N/A | ... | 0.19 | ... | -0.17 | 0.26 | 4.78 | Ti |
| Cr | N/A | ... | 0.03 | ... | -0.37 | 0.06 | 5.27 | Cr |
| Fe | N/A | -0.43 | ... | ... | -0.43 | ... | 7.07 | Fe |
| Ni | N/A | ... | 0.01 | ... | -0.39 | 0.04 | 5.83 | Ni |
Position
| Right Ascension : 11 08 40.07 | Declination : -44 15 33.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2002-12-07-0758 | N/A | VLT | 55000 | 330 | N/A | 159.2 |
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 | ... | -0.19 | ... | -0.66 | -0.23 | 4.77 | Mn |
| Fe | N/A | -0.43 | ... | ... | -0.43 | ... | 7.07 | Fe |
| Cu | N/A | ... | -0.01 | ... | -0.42 | 0.01 | 3.77 | Cu |
| Zn | N/A | ... | 0.18 | ... | -0.21 | 0.22 | 4.35 | Zn |
| Y | N/A | ... | 0.23 | ... | -0.17 | 0.26 | 2.04 | Y |
| Ba | N/A | ... | -0.08 | ... | -0.56 | -0.13 | 1.62 | Ba |
Position
| Right Ascension : 11 08 40.07 | Declination : -44 15 33.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2002-12-07-0758 | N/A | VLT | 55000 | 330 | N/A | 159.2 |