HE0430-4404: found in 2 paper(s).
Labels:
/P.S.Barklem et al.(2005)/
/S.Lucatello et al.(2006)/
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A0052
| Title | The Hamburg/ESO R-process enhanced star survey (HERES). II. Spectroscopic analysis of the survey sample |
| ADS | P.S.Barklem et al.,AAP, 439, 129, 2005 |
| Authors | P. S. Barklem, N. Christlieb, T. C. Beers, V. Hill, M. S. Bessell, J. Holmberg, B. Marsteller, S. Rossi, F. -J. Zickgraf, D. Reimers |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | N/A | VLT | 20000 | 49 | N/A | 201.5 |
Atmospheric data
| Teff | 6214 |
| log g | 4.27 |
| vturb | 1.41 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -0.80+-0.22 | 1.44+-0.26 | 7.75+-0.22 |
| Mg | ... | -1.79+-0.23 | 0.29+-0.23 | 5.79+-0.17 |
| Al | ... | -3.05+-0.22 | -0.97+-0.25 | 3.42+-0.22 |
| Ca | ... | -1.75+-0.20 | 0.33+-0.25 | 4.61+-0.20 |
| Sc | ... | -1.89+-0.26 | 0.19+-0.26 | 1.28+-0.23 |
| Ti | ... | -1.76+-0.25 | 0.32+-0.25 | 3.26+-0.21 |
| Cr | ... | -2.10+-0.21 | -0.02+-0.23 | 3.57+-0.21 |
| Mn | ... | -2.55+-0.24 | -0.47+-0.24 | 2.84+-0.20 |
| Fe | ... | -2.08+-0.17 | 0.00+-0.22 | 5.42+-0.17 |
| Co | ... | -1.98+-0.21 | 0.10+-0.25 | 2.94+-0.21 |
| Ni | ... | -2.07+-0.23 | 0.01+-0.23 | 4.18+-0.21 |
| Sr | ... | -1.52+-0.25 | 0.56+-0.25 | 1.45+-0.23 |
| Y | ... | -1.48+-0.26 | 0.60+-0.26 | 0.76+-0.23 |
| Ba | ... | -0.46+-0.18 | 1.62+-0.23 | 1.67+-0.18 |
| La | ... | -0.67+-0.26 | 1.41+-0.26 | 0.50+-0.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0120
| Title | The Frequency of Carbon-enhanced Metal-poor Stars in the Galaxy from the HERES Sample |
| ADS | S.Lucatello et al.,ApJ, 652, L37, 2006 |
| Authors | S. Lucatello, T. C. Beers, N. Christlieb, P. S. Barklem, S. Rossi, B. Marsteller, T. Sivarani, Y. S. Lee |
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Basic Informations
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -0.20 | 1.5 | 8.35 |
| N | ... | -0.90 | 0.8 | 7.07 |
| Fe | ... | -1.70 | ... | 5.80 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)