G94-49
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 : 5373 | log g : 4.5 | vturb : 1.1 |
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 | -0.8 | ... | ... | -0.80 | ... | 6.70 | Fe |
| Cu | N/A | ... | -0.06+-0.05 | ... | -0.84+-0.05 | -0.04+-0.05 | 3.35+-0.05 | Cu |
Position
| Right Ascension : 02 16 56.55 | Declination : +27 24 48.4 | 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 : 5373 | log g : 4.5 | vturb : 1.1 |
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 | ... | 0.06 | ... | -0.65 | 0.15 | 5.59 | Na |
| Mg | N/A | ... | 0.34 | ... | -0.48 | 0.32 | 7.12 | Mg |
| Si | N/A | ... | 0.32 | ... | -0.44 | 0.36 | 7.07 | Si |
| Ca | N/A | ... | 0.29 | ... | -0.49 | 0.31 | 5.85 | Ca |
| Ti | N/A | ... | 0.28 | ... | -0.45 | 0.35 | 4.50 | Ti |
| Cr | N/A | ... | 0.03 | ... | -0.74 | 0.06 | 4.90 | Cr |
| Fe | N/A | -0.80 | ... | ... | -0.80 | ... | 6.70 | Fe |
| Ni | N/A | ... | 0.01 | ... | -0.76 | 0.04 | 5.46 | Ni |
Position
| Right Ascension : 02 16 56.55 | Declination : +27 24 48.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-12-02-0030 | N/A | FIESNOT | 40000 | 170 | N/A | -163.9 |
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 | ... | -0.19 | ... | -1.03 | -0.23 | 4.40 | Mn |
| Fe | N/A | -0.8 | ... | ... | -0.80 | ... | 6.70 | Fe |
| Cu | N/A | ... | -0.05 | ... | -0.83 | -0.03 | 3.36 | Cu |
| Zn | N/A | ... | 0.21 | ... | -0.55 | 0.25 | 4.01 | Zn |
| Y | N/A | ... | 0.02 | ... | -0.75 | 0.05 | 1.46 | Y |
| Ba | N/A | ... | -0.14 | ... | -0.99 | -0.19 | 1.19 | Ba |
Position
| Right Ascension : 02 16 56.55 | Declination : +27 24 48.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-12-02-0030 | N/A | FIESNOT | 40000 | 170 | N/A | -163.9 |