G98-53
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 : 5848 | log g : 4.23 | 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 | -0.87 | ... | ... | -0.87 | ... | 6.63 | Fe |
| Cu | N/A | ... | -0.29+-0.04 | ... | -1.14+-0.04 | -0.27+-0.04 | 3.05+-0.04 | Cu |
Position
| Right Ascension : 06 13 49.83 | Declination : +33 25 02.1 | 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 : 5848 | log g : 4.23 | 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 | ... | -0.07 | ... | -0.85 | 0.02 | 5.39 | Na |
| Mg | N/A | ... | 0.2 | ... | -0.69 | 0.18 | 6.91 | Mg |
| Si | N/A | ... | 0.17 | ... | -0.66 | 0.21 | 6.85 | Si |
| Ca | N/A | ... | 0.25 | ... | -0.60 | 0.27 | 5.74 | Ca |
| Ti | N/A | ... | 0.12 | ... | -0.68 | 0.19 | 4.27 | Ti |
| Cr | N/A | ... | 0.01 | ... | -0.83 | 0.04 | 4.81 | Cr |
| Fe | N/A | -0.87 | ... | ... | -0.87 | ... | 6.63 | Fe |
| Ni | N/A | ... | -0.09 | ... | -0.93 | -0.06 | 5.29 | Ni |
Position
| Right Ascension : 06 13 49.83 | Declination : +33 25 02.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-12-04-1618 | N/A | FIESNOT | 40000 | 160 | N/A | 144.7 |
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 | ... | -0.30 | ... | -1.21 | -0.34 | 4.22 | Mn |
| Fe | N/A | -0.87 | ... | ... | -0.87 | ... | 6.63 | Fe |
| Cu | N/A | ... | -0.28 | ... | -1.13 | -0.26 | 3.06 | Cu |
| Zn | N/A | ... | 0.06 | ... | -0.77 | 0.10 | 3.79 | Zn |
| Y | N/A | ... | -0.06 | ... | -0.90 | -0.03 | 1.31 | Y |
| Ba | N/A | ... | -0.12 | ... | -1.04 | -0.17 | 1.14 | Ba |
Position
| Right Ascension : 06 13 49.83 | Declination : +33 25 02.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-12-04-1618 | N/A | FIESNOT | 40000 | 160 | N/A | 144.7 |