BPS BS16934-002: found in 2 paper(s).
Labels:
/W.Aoki et al.(2005)/
/W.Aoki et al.(2007)/
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A0057
| 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 |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-04-16 | N/A | SUBARUHDS | 50000 | 63 | 20min | +82.81+-0.26 |
| 2001-07-31 | N/A | SUBARUHDS | 50000 | 84 | 30min | +82.53+-0.26 |
| 2002-02-02 | N/A | SUBARUHDS | 50000 | 82 | 30min | +82.33+-0.21 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | +161539 |
| Right Ascension | 132946.4 |
Binarity
Photometric data
| V | 12.806 |
| B | 13.733 |
| H | 10.348 |
| J | 11.467 |
| K | 10.233 |
| EB-V | 0.00 |
Atmospheric data
| Teff | 4500 |
| log g | 1.0 |
| vturb | 2.0 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -3.09 | -0.3 | 5.3 |
| Mg I | ... | -1.54+-0.13 | 1.25+-0.13 | 6.04+-0.13 |
| Al I | ... | -2.76+-0.19 | 0.03+-0.19 | 3.73+-0.19 |
| Si I | ... | -2.55+-0.14 | 0.24+-0.14 | 5.01+-0.14 |
| Ca I | ... | -2.42+-0.13 | 0.37+-0.13 | 3.93+-0.13 |
| Sc II | ... | -2.09+-0.24 | 0.7+-0.24 | 1.01+-0.24 |
| Ti I | ... | -2.31+-0.13 | 0.48+-0.13 | 2.63+-0.13 |
| Ti II | ... | -2.09+-0.25 | 0.7+-0.25 | 2.85+-0.25 |
| Cr I | ... | -2.97+-0.11 | -0.18+-0.11 | 2.72+-0.11 |
| Mn I | ... | -3.52+-0.12 | -0.73+-0.12 | 2.01+-0.12 |
| Fe I | ... | -2.79+-0.21 | ... | 4.71+-0.21 |
| Fe II | ... | -2.81+-0.19 | ... | 4.69+-0.19 |
| Co I | ... | -2.50+-0.12 | 0.29+-0.12 | 2.41+-0.12 |
| Ni I | ... | -2.88+-0.12 | -0.09+-0.12 | 3.37+-0.12 |
| Zn I | ... | -2.75+-0.22 | 0.04+-0.22 | 1.92+-0.22 |
| Sr II | ... | -4.11+-0.25 | -1.32+-0.25 | -1.19+-0.25 |
| Y II | ... | -4.16+-0.25 | -1.37+-0.25 | -1.93+-0.25 |
| Zr II | ... | <-2.82 | <-0.03 | <-0.21 |
| Ba II | ... | -4.59+-0.22 | -1.8+-0.22 | -2.37+-0.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0117
| Title | Spectroscopic Studies of Extremely Metal-poor Stars with the Subaru High-Dispersion Spectrograph. IV. The alpha-Element–Enhanced Metal-poor Star BS 16934-002 |
| ADS | W.Aoki et al.,ApJ, 660, 747, 2007 |
| Authors | W. Aoki, S. Honda, T. C. Beers, M. Takada-Hidai, N. Iwamoto, N. Tominaga, H. Umeda, K. Nomoto, J. E. Norris, S. G. Ryan |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2004-03-31 | 2453158 | SUBARUHDS | 60000 | 100 | 7200 | 82.5+-0.3 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Atmospheric data
| Teff | 4500 |
| log g | 1.0 |
| vturb | 2.1 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -3.05+-0.17 | -0.27+-0.17 | 5.35+-0.17 |
| CN | ... | -2.13+-0.29 | +0.65+-0.29 | 5.65+-0.29 |
| O I | ... | -1.64+-0.19 | +1.14+-0.19 | 7.03+-0.19 |
| Na I | ... | -1.97+-0.13 | +0.81+-0.13 | 4.20+-0.13 |
| Mg I | ... | -1.55+-0.13 | +1.23+-0.13 | 5.98+-0.13 |
| Al I | ... | -2.61+-0.19 | +0.17+-0.19 | 3.76+-0.19 |
| Si I | ... | -2.34+-0.14 | +0.44+-0.14 | 5.17+-0.14 |
| Ca I | ... | -2.43+-0.13 | +0.35+-0.13 | 3.89+-0.13 |
| Sc II | ... | -2.19+-0.24 | +0.59+-0.24 | 0.87+-0.24 |
| Ti I | ... | -2.30+-0.13 | +0.48+-0.13 | 2.61+-0.13 |
| Ti II | ... | -2.16+-0.25 | +0.62+-0.25 | 2.74+-0.25 |
| Cr I | ... | -2.97+-0.11 | -0.19+-0.11 | 2.67+-0.11 |
| Mn I | ... | -3.39+-0.12 | -0.61+-0.12 | 2.01+-0.12 |
| Fe I | ... | -2.78+-0.20 | ... | 4.68+-0.20 |
| Fe II | ... | -2.79+-0.19 | ... | 4.67+-0.19 |
| Co I | ... | -2.59+-0.12 | +0.19+-0.12 | 2.34+-0.12 |
| Ni I | ... | -2.86+-0.12 | -0.08+-0.12 | 3.38+-0.12 |
| Zn I | ... | -2.67+-0.22 | +0.11+-0.22 | 1.94+-0.22 |
| Sr II | ... | -4.14+-0.25 | -1.36+-0.25 | -1.22+-0.25 |
| Ba II | ... | -4.47+-0.24 | -1.69+-0.24 | -2.29+-0.24 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)