BPS CS29526-110: found in 2 paper(s).
Labels:
/W.Aoki et al.(2002)/
/W.Aoki et al.(2002)/
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A0011
| Title | A SUBARU/HIGH DISPERSION SPECTROGRAPH STUDY OF LEAD (Pb) ABUNDANCES IN EIGHT s-PROCESS ELEMENT–RICH, METAL-POOR STARS |
| ADS | W.Aoki et al.,ApJ, 580, 1149, 2002 |
| Authors | W. Aoki, S. G. Ryan, J. E. Norris, T. C. Beers, H. Ando, S. Tsangarides |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-01-28 | 2451938 | SUBARUHDS | 50000 | 62 | 90*3 | 208.35+-0.76 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6500 |
| log g | 3.2 |
| vturb | 1.6 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Fe I | ... | -2.38+-0.16 | ... | 5.12+-0.16 |
| Fe II | ... | -2.38+-0.20 | ... | 5.12+-0.20 |
| Sr II | ... | -1.50+-0.43 | 0.88+-0.43 | 1.42+-0.43 |
| Zr II | ... | -1.27+-0.23 | 1.11+-0.23 | 1.34+-0.23 |
| Ba II | ... | -0.27+-0.17 | 2.11+-0.17 | 1.95+-0.17 |
| La II | ... | -0.69+-0.24 | 1.69+-0.24 | 0.53+-0.24 |
| Ce II | ... | -0.37+-0.22 | 2.01+-0.22 | 1.26+-0.22 |
| Nd II | ... | -0.37+-0.23 | 2.01+-0.23 | 1.12+-0.23 |
| Eu II | ... | -0.65+-0.20 | 1.73+-0.20 | -0.10+-0.20 |
| Pb II | ... | 0.92+-0.24 | 3.3+-0.24 | 3.0+-0.24 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0035
| Title | Subaru/HDS Study of the Extremely Metal-Poor Star CS 29498-043: Abundance Analysis Details and Comparison with Other Carbon-Rich Objects |
| ADS | W.Aoki et al.,, 54, 933, 2002 |
| Authors | W. Aoki, J. E. Norris, S. G. Ryan, T. C. Beers, H. Ando |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2451938 | SUBARUHDS | N/A | N/A | N/A | +208.35+-0.76 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6500 |
| log g | 3.2 |
| vturb | 1.6 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -0.18+-0.38 | +2.2+-0.38 | 8.37+-0.38 |
| CN | ... | -0.98 | +1.4 | 6.99 |
| Mg I | ... | -2.08+-0.19 | +0.30+-0.19 | 5.50+-0.19 |
| Al I | ... | -3.16+-0.16 | -0.78+-0.16 | 3.31+-0.16 |
| Si I | ... | -2.30+-0.10 | +0.08+-0.10 | 5.25+-0.10 |
| Ca I | ... | -2.02+-0.15 | +0.36+-0.15 | 4.34+-0.15 |
| Ti II | ... | -2.26+-0.22 | +0.12+-0.22 | 2.76+-0.22 |
| Cr I | ... | -2.71+-0.15 | -0.33+-0.15 | 2.96+-0.15 |
| Mn I | ... | -3.30+-0.10 | -0.92+-0.10 | 2.09+-0.10 |
| Fe I | ... | -2.38+-0.16 | ... | 5.12+-0.16 |
| Fe II | ... | -2.38+-0.20 | ... | 5.12+-0.20 |
| Ni I | ... | -2.49+-0.19 | -0.11+-0.19 | 3.76+-0.19 |
| Sr II | ... | -1.50+-0.43 | +0.88+-0.43 | 1.47+-0.43 |
| Ba II | ... | -0.27+-0.17 | +2.11+-0.17 | 1.86+-0.17 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)