G172-61
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 : 5225 | log g : 4.47 | vturb : 0.9 |
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 | -1 | ... | ... | -1.00 | ... | 6.50 | Fe |
| Cu | N/A | ... | -0.34+-0.03 | ... | -1.32+-0.03 | -0.32+-0.03 | 2.87+-0.03 | Cu |
Position
| Right Ascension : 01 34 22.69 | Declination : +48 44 27.5 | 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 : 5225 | log g : 4.47 | vturb : 0.9 |
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 | ... | -0.18 | ... | -1.09 | -0.09 | 5.15 | Na |
| Mg | N/A | ... | 0.16 | ... | -0.86 | 0.14 | 6.74 | Mg |
| Si | N/A | ... | 0.17 | ... | -0.79 | 0.21 | 6.72 | Si |
| Ca | N/A | ... | 0.26 | ... | -0.72 | 0.28 | 5.62 | Ca |
| Ti | N/A | ... | 0.16 | ... | -0.77 | 0.23 | 4.18 | Ti |
| Cr | N/A | ... | 0.04 | ... | -0.93 | 0.07 | 4.71 | Cr |
| Fe | N/A | -1.00 | ... | ... | -1.00 | ... | 6.50 | Fe |
| Ni | N/A | ... | -0.1 | ... | -1.07 | -0.07 | 5.15 | Ni |
Position
| Right Ascension : 01 34 22.69 | Declination : +48 44 27.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-11-30-2143 | N/A | FIESNOT | 40000 | 170 | N/A | -206.6 |
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 | ... | -0.26 | ... | -1.30 | -0.30 | 4.13 | Mn |
| Fe | N/A | -1 | ... | ... | -1.00 | ... | 6.50 | Fe |
| Cu | N/A | ... | -0.30 | ... | -1.28 | -0.28 | 2.91 | Cu |
| Zn | N/A | ... | 0.09 | ... | -0.87 | 0.13 | 3.69 | Zn |
| Y | N/A | ... | 0.11 | ... | -0.86 | 0.14 | 1.35 | Y |
| Ba | N/A | ... | -0.05 | ... | -1.10 | -0.10 | 1.08 | Ba |
Position
| Right Ascension : 01 34 22.69 | Declination : +48 44 27.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-11-30-2143 | N/A | FIESNOT | 40000 | 170 | N/A | -206.6 |