BPS CS22957-027: found in 4 paper(s).
Labels:
/W.Aoki et al.(2002)/
/W.Aoki et al.(2002)/
/G.W.Preston and C. Sneden(2001)/
/J.G.Cohen et al.(2006)/
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A0010
| Title | CHEMICAL COMPOSITION OF THE CARBON-RICH, EXTREMELY METAL POOR STAR CS 29498-043: A NEW CLASS OF EXTREMELY METAL POOR STARS WITH EXCESSES OF MAGNESIUM AND SILICON |
| ADS | W.Aoki et al.,ApJ, 576, L141, 2002 |
| Authors | W. Aoki, J. E. Norris, S. G. Ryan, T. C. Beers, H. Ando |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2001-07-23 | 2452114 | SUBARUHDS | 60000 | N/A | 4592 | -61.6+-0.22 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Binarity
Photometric data
| V | 13.59 |
| B | 11.61 |
| V-K | 0.74 |
| K | 1.92 |
Atmospheric data
| Teff | 5100 |
| log g | 1.9 |
| vturb | 1.4 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C2 | ... | -0.75+-0.24 | +2.37+-0.24 | 7.80+-0.24 |
| CN | ... | -1.50+-0.35 | +1.62+-0.35 | 6.45+-0.35 |
| Mg I | ... | -2.43+-0.20 | +0.69+-0.20 | 5.15+-0.20 |
| Al I | ... | -3.89+-0.33 | -0.77+-0.33 | 2.60+-0.33 |
| Ca I | ... | -2.98+-0.17 | +0.14+-0.17 | 3.37+-0.17 |
| Ti I | ... | -2.82+-0.11 | +0.30+-0.11 | 2.12+-0.11 |
| Ti II | ... | -2.71+-0.20 | +0.41+-0.20 | 2.23+-0.20 |
| Cr I | ... | -3.33+-0.11 | -0.21+-0.11 | 2.36+-0.11 |
| Mn I | ... | -3.53+-0.48 | -0.41+-0.48 | 2.0+-0.48 |
| Fe I | ... | -3.12+-0.15 | ... | 4.38+-0.15 |
| Fe II | ... | -3.11+-0.24 | ... | 4.39+-0.24 |
| Ni I | ... | -3.37+-0.26 | -0.25+-0.26 | 2.88+-0.26 |
| Sr II | ... | -3.68+-0.40 | -0.56+-0.40 | -0.76+-0.40 |
| Ba II | ... | -4.35+-0.21 | -1.23+-0.21 | -2.13+-0.21 |
: 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 |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2452114 | SUBARUHDS | N/A | N/A | N/A | -61.6+-0.22 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Binarity
Photometric data
Atmospheric data
| Teff | 5100 |
| log g | 1.9 |
| vturb | 1.4 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -0.72+-0.24 | +2.4+-0.24 | 7.83+-0.24 |
| CN | ... | -1.52 | +1.6 | 6.45 |
| Mg I | ... | -2.43+-0.20 | +0.69+-0.20 | 5.15+-0.20 |
| Al I | ... | -3.89+-0.33 | -0.77+-0.33 | 2.58+-0.33 |
| Ca I | ... | -2.98+-0.17 | +0.14+-0.17 | 3.38+-0.17 |
| Ti I | ... | -2.82+-0.11 | +0.30+-0.11 | 2.20+-0.11 |
| Ti II | ... | -2.71+-0.20 | +0.41+-0.20 | 2.31+-0.20 |
| Cr I | ... | -3.33+-0.11 | -0.21+-0.11 | 2.34+-0.11 |
| Mn I | ... | -3.53+-0.48 | -0.41+-0.48 | 1.86+-0.48 |
| Fe I | ... | -3.12+-0.15 | ... | 4.38+-0.15 |
| Fe II | ... | -3.11+-0.24 | ... | 4.39+-0.24 |
| Ni I | ... | -3.37+-0.26 | -0.25+-0.26 | 2.88+-0.26 |
| Sr II | ... | -3.68+-0.40 | -0.56+-0.40 | -0.71+-0.40 |
| Ba II | ... | -4.35+-0.21 | -1.23+-0.21 | -2.22+-0.21 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
A0044
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | 2448099.85 | FRUTTI | N/A | N/A | N/A | -70.0 |
| N/A | 2448114.86 | FRUTTI | N/A | N/A | N/A | -70.5 |
| N/A | 2448115.79 | FRUTTI | N/A | N/A | N/A | -69.6 |
| N/A | 2448116.80 | FRUTTI | N/A | N/A | N/A | -69.8 |
| N/A | 2448117.90 | FRUTTI | N/A | N/A | N/A | -71.0 |
| N/A | 2448119.84 | FRUTTI | N/A | N/A | N/A | -70.4 |
| N/A | 2451002.80 | FRUTTI | N/A | N/A | N/A | -63.7 |
| N/A | 2451035.76 | FRUTTI | N/A | N/A | N/A | -63.4 |
| N/A | 2451360.92 | FRUTTI | N/A | N/A | N/A | -70.1 |
| N/A | 2451384.82 | FRUTTI | N/A | N/A | N/A | -71.8 |
| N/A | 2451386.86 | FRUTTI | N/A | N/A | N/A | -72.6 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Binarity
| Binarity | Positive |
| Vrad | -72.8 |
| Period | 3125 |
Photometric data
Atmospheric data
| Teff | 5050 |
| log g | 2.0 |
| vturb | 2.0 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| CH | ... | -0.76 | 2.2 | 7.79 |
| CN | ... | -1.36 | 1.6 | 6.61 |
| Na I | ... | -2.19 | 0.77 | 4.14 |
| Mg I | ... | -2.75 | 0.21 | 4.83 |
| Ti II | ... | -2.81 | 0.15 | 2.21 |
| Fe I | ... | -2.96 | ... | 4.54 |
| Fe II | ... | -2.97 | ... | 4.53 |
| Sr II | ... | -3.66 | -0.7 | -0.69 |
| Ba II | ... | -4.96 | -2.0 | -2.83 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
A0090
| Title | Carbon Stars in the Hamburg/ESO Survey: Abundances |
| ADS | J.G.Cohen et al.,AJ, 132, 137, 2006 |
| Authors | J. G. Cohen, A. McWilliam, S. Shectman, I. Thompson, N. Christlieb, J. Melendez, S. Ramirez, A. Swensson, F. -J. Zickgraf |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | KECKHIRES | 45000 | 100 | 6000 | |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -035349 |
| Right Ascension | 235913.1 |
Binarity
Photometric data
Atmospheric data
| Teff | 5205 |
| log g | 2.5 |
| vturb | 1.8 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| CH | ... | -0.93 | 2.14 | 7.66 |
| CN | ... | -1.18 | 1.89 | 6.75 |
| Mg I | ... | -2.71+-0.50 | 0.36+-0.50 | 4.83+-0.50 |
| Al I | ... | -2.82 | 0.25 | 3.65 |
| Ca I | ... | -2.36+-0.13 | 0.71+-0.13 | 4.01+-0.13 |
| Sc II | ... | -2.59 | 0.48 | 0.51 |
| Ti I | ... | -2.82+-0.13 | 0.25+-0.13 | 2.17+-0.13 |
| Ti II | ... | -2.74+-0.23 | 0.33+-0.23 | 2.25+-0.23 |
| Cr I | ... | -3.43 | -0.36 | 2.24 |
| Mn I | ... | -3.17+-0.28 | -0.10+-0.28 | 2.22+-0.28 |
| Fe I | ... | -3.07+-0.21 | ... | 4.38+-0.21 |
| Fe II | ... | -3.18+-0.15 | -0.06+-0.15 | 4.32+-0.15 |
| Co I | ... | -2.89 | 0.18 | 2.03 |
| Zn I | ... | -2.56 | 0.51 | 2.04 |
| Sr II | ... | -4.05 | -0.98 | -1.15 |
| Y II | ... | <-3.08+-0.25 | <-0.01+-0.25 | <-0.84+-0.25 |
| Ba II | ... | -3.85+-0.25 | -0.78+-0.25 | -1.72+-0.25 |
| La II | ... | <-2.47 | <0.60 | <-1.33 |
| Ce II | ... | <-2.03 | <1.04 | <-0.48 |
| Nd II | ... | <-1.87+-0.26 | <1.20+-0.26 | <-0.36+-0.26 |
| Eu II | ... | <-2.10+-0.35 | <0.97+-0.35 | <-1.59+-0.35 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)