HD59392
taken from 3 paper(s):
/M.Asplund et al.(2006)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Lithium Isotopic Abundances in Metal-poor Halo Stars
Stellar Parameters
| Teff : 5936 | log g : 3.99 | vturb : 1.5 |
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 |
|---|
| Li | N/A | ... | ... | 2.24+-0.01 | -1.02+-0.01 | 0.59+-0.01 | 2.24+-0.01 | Li |
| O | N/A | -1.04 | ... | ... | -0.99 | 0.62 | 7.70 | O |
| Fe | N/A | -1.61 | ... | ... | -1.61 | ... | 5.89 | Fe |
Isotopic Ratio
Binary Parameters
Position
| Right Ascension : 07 28 03.22 | Declination : -38 00 41.3 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2002-02-05-0253 | N/A | VLT | 120000 | 710 | 60 | 267.9 |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
| Teff : 6012 | log g : 3.91 | vturb : 1.9 |
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 | ... | -0.15 | ... | -1.66 | -0.06 | 4.58 | Na |
| Mg | N/A | ... | 0.28 | ... | -1.34 | 0.26 | 6.26 | Mg |
| Si | N/A | ... | 0.27 | ... | -1.29 | 0.31 | 6.22 | Si |
| Ca | N/A | ... | 0.38 | ... | -1.20 | 0.40 | 5.14 | Ca |
| Ti | N/A | ... | 0.33 | ... | -1.20 | 0.40 | 3.75 | Ti |
| Cr | N/A | ... | 0.00 | ... | -1.57 | 0.03 | 4.07 | Cr |
| Fe | N/A | -1.60 | ... | ... | -1.60 | ... | 5.90 | Fe |
| Ni | N/A | ... | -0.01 | ... | -1.58 | 0.02 | 4.64 | Ni |
Position
| Right Ascension : 07 28 03.22 | Declination : -38 00 41.3 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-03-07-0353 | N/A | VLT | 55000 | 410 | N/A | 268.4 |
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 | ... | -0.36 | ... | -2.00 | -0.40 | 3.43 | Mn |
| Fe | N/A | -1.60 | ... | ... | -1.60 | ... | 5.90 | Fe |
| Zn | N/A | ... | 0.14 | ... | -1.42 | 0.18 | 3.14 | Zn |
| Y | N/A | ... | 0.13 | ... | -1.44 | 0.16 | 0.77 | Y |
| Ba | N/A | ... | -0.07 | ... | -1.72 | -0.12 | 0.46 | Ba |
Position
| Right Ascension : 07 28 03.22 | Declination : -38 00 41.3 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-03-07-0353 | N/A | VLT | 55000 | 410 | N/A | 268.4 |