HD177095
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 : 5349 | log g : 4.39 | 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 | -0.74 | ... | ... | -0.74 | ... | 6.76 | Fe |
| Cu | N/A | ... | -0.12+-0.04 | ... | -0.84+-0.04 | -0.10+-0.04 | 3.35+-0.04 | Cu |
Position
| Right Ascension : 19 03 56.71 | Declination : -20 27 36.6 | 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 : 5349 | log g : 4.39 | 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 | ... | 0.05 | ... | -0.60 | 0.14 | 5.64 | Na |
| Mg | N/A | ... | 0.38 | ... | -0.38 | 0.36 | 7.22 | Mg |
| Si | N/A | ... | 0.3 | ... | -0.40 | 0.34 | 7.11 | Si |
| Ca | N/A | ... | 0.31 | ... | -0.41 | 0.33 | 5.93 | Ca |
| Ti | N/A | ... | 0.28 | ... | -0.39 | 0.35 | 4.56 | Ti |
| Cr | N/A | ... | 0.02 | ... | -0.69 | 0.05 | 4.95 | Cr |
| Fe | N/A | -0.74 | ... | ... | -0.74 | ... | 6.76 | Fe |
| Ni | N/A | ... | 0.01 | ... | -0.70 | 0.04 | 5.52 | Ni |
Position
| Right Ascension : 19 03 56.71 | Declination : -20 27 36.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-05-19-0404 | N/A | FIESNOT | 40000 | 160 | N/A | 90.8 |
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 | ... | -0.24 | ... | -1.02 | -0.28 | 4.41 | Mn |
| Fe | N/A | -0.74 | ... | ... | -0.74 | ... | 6.76 | Fe |
| Cu | N/A | ... | -0.10 | ... | -0.82 | -0.08 | 3.37 | Cu |
| Zn | N/A | ... | 0.19 | ... | -0.51 | 0.23 | 4.05 | Zn |
| Y | N/A | ... | 0.06 | ... | -0.65 | 0.09 | 1.56 | Y |
| Ba | N/A | ... | -0.03 | ... | -0.82 | -0.08 | 1.36 | Ba |
Position
| Right Ascension : 19 03 56.71 | Declination : -20 27 36.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-05-19-0404 | N/A | FIESNOT | 40000 | 160 | N/A | 90.8 |