BPS CS29526-110: found in 3 paper(s).
Labels:
/W.Aoki et al.(2002)/
/W.Aoki et al.(2002)/
/W.Aoki et al.(2008)/
Find this object in SIMBAD
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 |
Get more information of this paper.
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 |
Binarity
Photometric data
| V | 13.37 |
| B-V | 0.35 |
| EB-V | 0.00 |
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 |
Binarity
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)
A0174
| Title | Carbon-Enhanced Metal-Poor Stars. III. Main-Sequence Turnoff Stars from the SDSS SEGUE Sample |
| ADS | W.Aoki et al.,ApJ, 678, 1351, 2008 |
| Authors | W. Aoki, T. C. Beers, T. Sivarani, B. Marsteller, Y. S. Lee, S. Honda, J. E. Norris, S. G. Ryan, D. Carollo |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2007-02-10 | 2454141.72 | SUBARUHDS | 45000 | N/A | 40 | 203.09+-0.39 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
| V | 13.352 |
| B-V | 0.356 |
| K | 12.367 |
| EB-V | 0.033 |
Atmospheric data
| Teff | 6800+-150 |
| log g | 4.1+-0.3 |
| vturb | 2.1+-0.3 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li | ... | <1.14 | <3.20 | <2.3 |
| C | ... | 0.01+-0.26 | 2.07+-0.26 | 8.4+-0.26 |
| Na I | ... | -1.92+-0.19 | 0.14+-0.19 | 4.25+-0.19 |
| Mg I | ... | -1.84+-0.16 | 0.22+-0.16 | 5.69+-0.16 |
| Ca I | ... | -1.87+-0.10 | 0.19+-0.10 | 4.45+-0.10 |
| Ti II | ... | -1.82+-0.14 | 0.24+-0.14 | 3.08+-0.14 |
| Cr I | ... | -2.11+-0.11 | -0.05+-0.11 | 3.53+-0.11 |
| Fe I | ... | -2.06+-0.11 | ... | 5.39+-0.11 |
| Fe II | ... | -2.07+-0.12 | ... | 5.38+-0.12 |
| Ni I | ... | -1.71+-0.11 | 0.35+-0.11 | 4.52+-0.11 |
| Sr II | ... | -1.29+-0.27 | 0.77+-0.27 | 1.63+-0.27 |
| Y II | ... | -0.72+-0.20 | 1.34+-0.20 | 1.50+-0.20 |
| Zr II | ... | -0.80+-0.20 | 1.26+-0.20 | 1.80+-0.20 |
| Ba II | ... | 0.33+-0.22 | 2.39+-0.22 | 2.5+-0.22 |
| La II | ... | 0.03+-0.20 | 2.09+-0.20 | 1.16+-0.20 |
| Pb I | ... | 1.10 | 3.16 | 3.1 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)