HE1300-2201: 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 | 52 | N/A | -62.8 |
Atmospheric data
| Teff | 6332 |
| log g | 4.64 |
| vturb | 1.34 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -1.75+-0.23 | 1.01+-0.27 | 6.80+-0.23 |
| Mg | ... | -2.31+-0.24 | 0.29+-0.24 | 5.27+-0.18 |
| Al | ... | -3.52+-0.21 | -0.92+-0.25 | 2.95+-0.21 |
| Ca | ... | -2.31+-0.20 | 0.29+-0.25 | 4.05+-0.20 |
| Sc | ... | -2.41+-0.27 | 0.19+-0.27 | 0.76+-0.23 |
| Ti | ... | -2.22+-0.26 | 0.38+-0.26 | 2.80+-0.22 |
| Cr | ... | -2.70+-0.19 | -0.11+-0.23 | 2.97+-0.19 |
| Fe | ... | -2.60+-0.17 | 0.00+-0.22 | 4.90+-0.17 |
| Co | ... | -2.20+-0.21 | 0.39+-0.25 | 2.72+-0.21 |
| Ni | ... | -2.67+-0.23 | -0.07+-0.23 | 3.58+-0.19 |
| Sr | ... | -2.32+-0.28 | 0.28+-0.28 | 0.65+-0.27 |
| Ba | ... | -2.64+-0.23 | -0.04+-0.27 | -0.51+-0.23 |
: 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 | ... | -0.41 | 1.9 | 8.14 |
| N | ... | -0.81 | 1.5 | 7.16 |
| Fe | ... | -2.31 | ... | 5.19 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)