HE1523-1155: found in 2 paper(s).
Labels:
/S.Lucatello et al.(2006)/
/W.Aoki et al.(2007)/
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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 | ... | -0.54 | 1.6 | 8.01 |
| N | ... | -0.64 | 1.5 | 7.33 |
| Fe | ... | -2.14 | ... | 5.36 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0122
| Title | Carbon-enhanced Metal-poor Stars. I. Chemical Compositions of 26 Stars |
| ADS | W.Aoki et al.,ApJ, 655, 492, 2007 |
| Authors | W. Aoki, T. Beers, N. Christlieb, J. E. Norris, S. G. Ryan, S. Tsangarides |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2003-05-26 | N/A | SUBARUHDS | 50000 | N/A | 600 | -45.03+-0.12 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -120543 |
| Right Ascension | 152641.0 |
Photometric data
| V | 13.225 |
| B | 14.571 |
| H | 10.846 |
| J | 11.372 |
| K | 10.748 |
| EB-V | 0.05 |
Atmospheric data
| Teff | 4800 |
| log g | 1.6 |
| vturb | 1.8 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -0.29+-0.19 | 1.86+-0.19 | 8.1+-0.19 |
| N | ... | -0.48+-0.52 | 1.67+-0.52 | 7.3+-0.52 |
| Mg | ... | -1.53+-0.15 | 0.62+-0.15 | 6.00+-0.15 |
| Ca | ... | -1.69+-0.11 | 0.46+-0.11 | 4.63+-0.11 |
| Ti I | ... | -1.83+-0.11 | 0.32+-0.11 | 3.07+-0.11 |
| Ti II | ... | -1.88+-0.17 | 0.27+-0.17 | 3.02+-0.17 |
| Fe I | ... | -2.15+-0.19 | ... | 5.30+-0.19 |
| Fe II | ... | -2.17+-0.14 | ... | 5.28+-0.14 |
| Ba | ... | -0.43+-0.14 | 1.72+-0.14 | 1.74+-0.14 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)