BPS CS22960-053: 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 |
|---|
| 2003-09-06 | N/A | RCCTIO | N/A | 40 | 3600 | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
| V | 14.830 |
| B-V | 0.760 |
| U-B | 0.100 |
| V-K | 2.069 |
| EB-V | 0.01 |
Atmospheric data
| Teff | 5061 |
| log g | 2.38 |
| vturb | 1.68 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -1.93+-0.29 | +1.15+-0.29 | 6.63+-0.25 |
| N | ... | -1.93+-0.25 | +1.15+-0.25 | 6.12+-0.25 |
| Fe | ... | -3.08+-0.21 | ... | 4.42+-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 | 2400 | 282.26+-0.08 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -435421 |
| Right Ascension | 221617.0 |
Binarity
Photometric data
| V | 14.950 |
| B | 15.705 |
| H | 12.833 |
| J | 13.298 |
| K | 12.761 |
| EB-V | 0.07 |
Atmospheric data
| Teff | 5200 |
| log g | 2.1 |
| vturb | 2.1 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -1.09+-0.16 | 2.05+-0.16 | 7.3+-0.16 |
| CN | ... | -0.08+-0.21 | 3.06+-0.21 | 7.7+-0.21 |
| Mg I | ... | -2.49+-0.12 | 0.65+-0.12 | 5.04+-0.12 |
| Ca I | ... | -2.71+-0.12 | 0.43+-0.12 | 3.61+-0.12 |
| Sc II | ... | -2.65+-0.15 | 0.49+-0.15 | 0.40+-0.15 |
| Ti II | ... | -2.60+-0.15 | 0.54+-0.15 | 2.30+-0.15 |
| Cr I | ... | -3.37+-0.11 | -0.23+-0.11 | 2.27+-0.11 |
| Fe I | ... | -3.14+-0.15 | ... | 4.31+-0.15 |
| Fe II | ... | -3.15+-0.15 | ... | 4.30+-0.15 |
| Ba II | ... | -2.28+-0.14 | 0.86+-0.14 | -0.11+-0.14 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)