HE2330-0555: 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 | ... | -0.80 | 2.0 | 7.75 |
| N | ... | -1.90 | 0.9 | 6.07 |
| Fe | ... | -2.80 | ... | 4.70 |
: 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 | 1200 | -235.03+-0.09 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -053850 |
| Right Ascension | 233254.8 |
Photometric data
| V | 14.559 |
| B | 15.412 |
| H | 12.395 |
| J | 12.850 |
| K | 12.300 |
| EB-V | 0.03 |
Atmospheric data
| Teff | 4900 |
| log g | 1.7 |
| vturb | 1.8 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -0.69+-0.19 | 2.09+-0.19 | 7.7+-0.19 |
| N | ... | -1.78+-0.42 | 1.00+-0.42 | 6.0+-0.42 |
| Na | ... | -1.81+-0.12 | 0.97+-0.12 | 4.37+-0.12 |
| Mg | ... | -2.11+-0.17 | 0.67+-0.17 | 5.42+-0.17 |
| Ca | ... | -2.36+-0.19 | 0.42+-0.19 | 3.96+-0.19 |
| Sc | ... | -2.53+-0.08 | 0.25+-0.08 | 0.53+-0.08 |
| Ti I | ... | -2.47+-0.11 | 0.31+-0.11 | 2.44+-0.11 |
| Ti II | ... | -2.39+-0.23 | 0.39+-0.23 | 2.51+-0.23 |
| Cr | ... | -2.88+-0.10 | -0.10+-0.10 | 2.77+-0.10 |
| Fe I | ... | -2.78+-0.19 | ... | 4.68+-0.19 |
| Fe II | ... | -2.76+-0.14 | ... | 4.69+-0.14 |
| Ba | ... | -1.56+-0.25 | 1.22+-0.25 | 0.61+-0.25 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)