HE1351-1049: 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 | 45 | N/A | 285.4 |
Atmospheric data
| Teff | 5204 |
| log g | 2.85 |
| vturb | 1.48 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -2.06+-0.26 | 1.55+-0.28 | 6.49+-0.26 |
| Mg | ... | -3.15+-0.27 | 0.30+-0.27 | 4.43+-0.21 |
| Al | ... | -4.22+-0.22 | -0.77+-0.25 | 2.25+-0.22 |
| Ca | ... | -3.13+-0.21 | 0.32+-0.25 | 3.23+-0.21 |
| Sc | ... | -3.17+-0.25 | 0.28+-0.25 | 0.00+-0.24 |
| Ti | ... | -3.15+-0.25 | 0.30+-0.25 | 1.87+-0.22 |
| Cr | ... | -3.73+-0.22 | -0.28+-0.24 | 1.94+-0.22 |
| Mn | ... | -4.08+-0.24 | -0.63+-0.24 | 1.32+-0.21 |
| Fe | ... | -3.45+-0.18 | 0.00+-0.22 | 4.05+-0.18 |
| Co | ... | -2.97+-0.22 | 0.48+-0.25 | 1.95+-0.22 |
| Ni | ... | -3.15+-0.23 | 0.30+-0.23 | 3.10+-0.23 |
| Sr | ... | -3.42+-0.30 | 0.03+-0.30 | -0.45+-0.32 |
| Ba | ... | -3.31+-0.24 | 0.13+-0.25 | -1.18+-0.24 |
: 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 | ... | -1.33 | 1.6 | 7.22 |
| N | ... | -1.73 | 1.2 | 6.24 |
| Fe | ... | -2.93 | ... | 4.57 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)