BPS CS30301-015: 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 |
2001-07Y-25 | 2452116 | SUBARUHDS | 50000 | 53 | 50*2 | 86.46+-0.43 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4750 |
log g | 0.8 |
vturb | 2.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -2.64+-0.18 | ... | 4.86+-0.18 |
Fe II | ... | -2.63+-0.15 | ... | 4.87+-0.15 |
Sr II | ... | -2.34+-0.23 | 0.3+-0.23 | 0.6+-0.23 |
Y II | ... | -2.35+-0.20 | 0.29+-0.20 | -0.12+-0.20 |
Ba II | ... | -1.19+-0.16 | 1.45+-0.16 | 1.03+-0.16 |
La II | ... | -1.80+-0.25 | 0.84+-0.25 | -0.58+-0.25 |
Ce II | ... | -1.48+-0.15 | 1.16+-0.15 | 0.15+-0.15 |
Nd II | ... | -1.39+-0.17 | 1.25+-0.17 | -0.42+-0.17 |
Sm II | ... | -1.79+-0.20 | 0.85+-0.20 | -0.81+-0.20 |
Eu II | ... | -2.44+-0.18 | 0.2+-0.18 | -1.9+-0.18 |
Dy II | ... | -2.07+-0.20 | 0.57+-0.20 | -0.90+-0.20 |
Pb II | ... | -0.94+-0.24 | 1.7+-0.24 | 1.1+-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 |
| 2452116 | SUBARUHDS | N/A | N/A | N/A | +86.46+-0.43 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
Atmospheric data
Teff | 4750 |
log g | 0.8 |
vturb | 2.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -1.04+-0.28 | +1.6+-0.28 | 7.51+-0.28 |
CN | ... | -0.94 | +1.7 | 7.03 |
Mg I | ... | -1.78+-0.22 | +0.86+-0.22 | 5.80+-0.22 |
Al I | ... | -2.49 | +0.15 | 3.98 |
Ca I | ... | -1.87+-0.16 | +0.77+-0.16 | 4.49+-0.16 |
Ti I | ... | -2.41+-0.13 | +0.23+-0.13 | 2.61+-0.13 |
Ti II | ... | -2.26+-0.24 | +0.38+-0.24 | 2.76+-0.24 |
Fe I | ... | -2.64+-0.18 | ... | 4.86+-0.18 |
Fe II | ... | -2.63+-0.15 | ... | 4.87+-0.15 |
Zn I | ... | -2.31 | +0.33 | 2.29 |
Sr II | ... | -2.34 | +0.3 | 0.63 |
Ba II | ... | -1.19+-0.16 | +1.45+-0.16 | 0.94+-0.16 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio