BPS CS22174-007: found in 2 paper(s).
Labels:
/J.A.Johnson et al.(2007)/
/W.Aoki et al.(2007)/
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A0114
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2003-08-30 | N/A | RCCTIO | N/A | 142 | 5400 | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
| V | 12.409 |
| B-V | 0.694 |
| V-R | 0.448 |
| V-K | 2.091 |
| EB-V | 0.03 |
Atmospheric data
| Teff | 5059 |
| log g | 2.37 |
| vturb | 1.69 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -2.40+-0.29 | -0.40+-0.29 | 6.16+-0.25 |
| N | ... | <-2.89+-0.25 | <-0.89+-0.25 | <5.16+-0.25 |
| Fe | ... | -2.00+-0.21 | ... | 5.50+-0.21 |
: 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 | 600 | -70.76+-0.03 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -110232 |
| Right Ascension | 011406.7 |
Binarity
Photometric data
| V | 12.409 |
| B | 13.103 |
| H | 10.404 |
| J | 10.885 |
| K | 10.318 |
| EB-V | 0.08 |
Atmospheric data
| Teff | 5300 |
| log g | 2.7 |
| vturb | 2.1 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -1.79+-0.16 | 0.41+-0.16 | 6.6+-0.16 |
| CN | ... | <-0.78+-0.07 | <1.42+-0.07 | <7.0+-0.07 |
| Na I | ... | -1.90+-0.17 | 0.30+-0.17 | 4.27+-0.17 |
| Mg I | ... | -1.71+-0.10 | 0.49+-0.10 | 5.82+-0.10 |
| Ca I | ... | -1.96+-0.10 | 0.24+-0.10 | 4.35+-0.10 |
| Sc II | ... | -2.09+-0.14 | 0.11+-0.14 | 0.96+-0.14 |
| Ti I | ... | -1.81+-0.09 | 0.39+-0.09 | 3.09+-0.09 |
| Ti II | ... | -1.74+-0.14 | 0.46+-0.14 | 3.17+-0.14 |
| Cr I | ... | -2.39+-0.09 | -0.19+-0.09 | 3.26+-0.09 |
| Fe I | ... | -2.20+-0.14 | ... | 5.26+-0.14 |
| Fe II | ... | -2.20+-0.13 | ... | 5.26+-0.13 |
| Ni I | ... | -2.17+-0.11 | 0.03+-0.11 | 4.07+-0.11 |
| Zn I | ... | -2.14+-0.13 | 0.06+-0.13 | 2.46+-0.13 |
| Ba II | ... | -2.77+-0.13 | -0.57+-0.13 | -0.59+-0.13 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)