HE0400-2030: 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 | ... | -0.90 | 1.0 | 7.65 |
| N | ... | 0.60 | 2.5 | 8.57 |
| Fe | ... | -1.90 | ... | 5.60 |
: 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 |
| 2002-10-26 | N/A | SUBARUHDS | 50000 | N/A | 900 | 221.83+-0.05 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -202153 |
| Right Ascension | 040214.8 |
Photometric data
| V | 14.033 |
| B | 14.921 |
| H | 12.064 |
| J | 12.494 |
| K | 11.975 |
| EB-V | 0.13 |
Atmospheric data
| Teff | 5600 |
| log g | 3.5 |
| vturb | 2.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -0.59+-0.16 | 1.14+-0.16 | 7.8+-0.16 |
| N | ... | 1.02+-0.31 | 2.75+-0.31 | 8.8+-0.31 |
| Na | ... | -1.02+-0.20 | 0.71+-0.20 | 5.15+-0.20 |
| Mg | ... | -1.11+-0.14 | 0.62+-0.14 | 6.42+-0.14 |
| Ca | ... | -1.55+-0.14 | 0.18+-0.14 | 4.76+-0.14 |
| Sc | ... | -1.41+-0.17 | 0.32+-0.17 | 1.63+-0.17 |
| Ti I | ... | -1.46+-0.14 | 0.27+-0.14 | 3.44+-0.14 |
| Ti II | ... | -1.32+-0.17 | 0.41+-0.17 | 3.58+-0.17 |
| Cr | ... | -1.81+-0.14 | -0.08+-0.14 | 3.82+-0.14 |
| Fe I | ... | -1.73+-0.17 | ... | 5.72+-0.17 |
| Fe II | ... | -1.76+-0.18 | ... | 5.70+-0.18 |
| Ni | ... | -1.83+-0.15 | -0.10+-0.15 | 4.40+-0.15 |
| Zn | ... | -1.93+-0.16 | -0.20+-0.16 | 2.67+-0.16 |
| Ba | ... | -0.09+-0.16 | 1.64+-0.16 | 2.07+-0.16 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)