BPS BS17439-065: found in 1 paper(s).
Labels:| Title | Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements |
| ADS | W.Aoki et al.,ApJ, 632, 611, 2005 |
| Authors | W. Aoki, S. Honda, T. C. Beers, T. Kajino, H. Ando, J. E. Norris, S. G. Ryan, H. Izumiura, K. Sadakane, M. Takada-Hidai |
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| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2002-02-02 | N/A | SUBARUHDS | 50000 | 130 | 60min | +372.21+-0.30 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -133840 |
| Right Ascension | 110120.2 |
| V | 13.434 |
| B | 14.141 |
| H | 11.438 |
| J | 11.880 |
| K | 11.370 |
| EB-V | 0.02 |
| Teff | 5100 |
| log g | 1.6 |
| vturb | 2.3 |
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|---|---|---|---|
| C | ... | -2.89 | -0.5 | 5.5 |
| Mg | ... | -1.85+-0.10 | 0.54+-0.10 | 5.73+-0.10 |
| Al | ... | -3.26+-0.17 | -0.87+-0.17 | 3.23+-0.17 |
| Si | ... | -2.13+-0.12 | 0.26+-0.12 | 5.43+-0.12 |
| Ca | ... | -2.14+-0.10 | 0.25+-0.10 | 4.21+-0.10 |
| Sc | ... | -2.31+-0.23 | 0.08+-0.23 | 0.79+-0.23 |
| Ti I | ... | -2.10+-0.11 | 0.29+-0.11 | 2.84+-0.11 |
| Ti II | ... | -1.95+-0.24 | 0.44+-0.24 | 2.99+-0.24 |
| Cr | ... | -2.77+-0.09 | -0.38+-0.09 | 2.92+-0.09 |
| Mn | ... | -3.10+-0.19 | -0.71+-0.19 | 2.43+-0.19 |
| Fe I | ... | -2.39+-0.20 | ... | 5.11+-0.20 |
| Fe II | ... | -2.37+-0.18 | ... | 5.13+-0.18 |
| Co | ... | -2.13+-0.11 | 0.26+-0.11 | 2.78+-0.11 |
| Ni | ... | -2.38+-0.10 | 0.01+-0.10 | 3.87+-0.10 |
| Zn | ... | -2.33+-0.21 | 0.06+-0.21 | 2.34+-0.21 |
| Sr | ... | -2.66+-0.23 | -0.27+-0.23 | 0.26+-0.23 |
| Y | ... | -2.81+-0.08 | -0.42+-0.08 | -0.58+-0.08 |
| Zr | ... | -2.33+-0.08 | 0.06+-0.08 | 0.28+-0.08 |
| Ba | ... | -2.85+-0.21 | -0.46+-0.21 | -0.63+-0.21 |
| La | ... | -2.13+-0.24 | 0.26+-0.24 | -1.33+-0.24 |
| Nd | ... | -2.47+-0.24 | -0.08+-0.24 | -0.98+-0.24 |
| Eu | ... | -2.30+-0.24 | 0.09+-0.24 | -1.75+-0.24 |
| Gd | ... | -2.47+-0.18 | -0.08+-0.18 | -1.38+-0.18 |
| Dy | ... | -1.92+-0.19 | 0.47+-0.19 | -0.75+-0.19 |