G150-40
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 : 5968 | log g : 4.09 | vturb : 1.4 |
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 | -0.81 | ... | ... | -0.81 | ... | 6.69 | Fe |
| Cu | N/A | ... | -0.34+-0.00 | ... | -1.13+-0.00 | -0.32+-0.00 | 3.06+-0.00 | Cu |
Position
| Right Ascension : 13 48 52.14 | Declination : +27 40 09.6 | 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 : 5968 | log g : 4.09 | vturb : 1.4 |
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 | ... | 0.28 | ... | -0.44 | 0.37 | 5.80 | Na |
| Mg | N/A | ... | 0.14 | ... | -0.69 | 0.12 | 6.91 | Mg |
| Si | N/A | ... | 0.19 | ... | -0.58 | 0.23 | 6.93 | Si |
| Ca | N/A | ... | 0.19 | ... | -0.60 | 0.21 | 5.74 | Ca |
| Ti | N/A | ... | 0.12 | ... | -0.62 | 0.19 | 4.33 | Ti |
| Cr | N/A | ... | 0.01 | ... | -0.77 | 0.04 | 4.87 | Cr |
| Fe | N/A | -0.81 | ... | ... | -0.81 | ... | 6.69 | Fe |
| Ni | N/A | ... | -0.08 | ... | -0.86 | -0.05 | 5.36 | Ni |
Position
| Right Ascension : 13 48 52.14 | Declination : +27 40 09.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-05-17-0810 | N/A | FIESNOT | 40000 | 170 | N/A | -50.5 |
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 | ... | -0.20 | ... | -1.05 | -0.24 | 4.38 | Mn |
| Fe | N/A | -0.81 | ... | ... | -0.81 | ... | 6.69 | Fe |
| Cu | N/A | ... | -0.28 | ... | -1.07 | -0.26 | 3.12 | Cu |
| Zn | N/A | ... | 0.01 | ... | -0.76 | 0.05 | 3.80 | Zn |
| Y | N/A | ... | -0.16 | ... | -0.94 | -0.13 | 1.27 | Y |
| Ba | N/A | ... | -0.13 | ... | -0.99 | -0.18 | 1.19 | Ba |
Position
| Right Ascension : 13 48 52.14 | Declination : +27 40 09.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-05-17-0810 | N/A | FIESNOT | 40000 | 170 | N/A | -50.5 |