BPS CS29497-034: found in 4 paper(s).
Labels:
/V.Hill et al.(2000)/
/B.Barbuy et al.(2005)/
/A.Frebel et al.(2006)/
/W.Aoki et al.(2007)/
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A0032
| Title | Heavy-element abundances in the CH/CN-strong very metal-poor stars CS 22948-27 and CS 29497-34 |
| ADS | V.Hill et al.,AAP, 353, 557, 2000 |
| Authors | V. Hill, B. Barbuy, M. Spite, F. Spite, R. Cayrel, B. Plez, T. C. Department of Physics andtronomy, MSU. Beers, B. Nordstrom, P. E. Institute of Physics and Astronomy, AarhusU. Nissen |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 1995-09-14 | N/A | EMMIESO | 30000 | 175 | 95min | -44.7 |
| 1995-09-14 | N/A | EMMIESO | 30000 | 220 | 120min | -44.6 |
| 1995-11-03 | N/A | EMMIESO | 30000 | 90 | 90min | -46.6 |
| 1995-11-04 | N/A | EMMIESO | 30000 | 76 | 75min | -45.7 |
| 1996-10-01 | N/A | CASPECESO | 21000 | 170 | 120min | -43.3 |
| 1996-10-02 | N/A | CASPECESO | 21000 | 190 | 120min | -42.2 |
| 1999-07-03 | N/A | FEROSESO | 48000 | 35 | 30min | -44.7 |
| Galactic Longitude (l) | 52.81 |
| Galactic Latitude (b) | -87.67 |
| Declination | -26 18 55 |
| Right Ascension | 00h41m39.9s |
Photometric data
| V | 12.20 |
| B-V | 1.10+-0.016 |
| V-R | 0.48+-0.015 |
| R-I | 0.42+-0.005 |
| EB-V | 0.01 |
Atmospheric data
| Teff | 4800 |
| log g | 1.80 |
| vturb | 1.50 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| CH | ... | -0.55 | +2.35 | 8.00 |
| C2 | ... | -0.40 | +2.5 | 8.15 |
| CN | ... | -0.60 | +2.3 | 7.37 |
| Na | ... | -1.60 | +1.30 | 4.73 |
| Mg | ... | -2.28 | +0.62 | 5.30 |
| Fe I | ... | -2.90 | ... | 4.60 |
| Fe II | ... | -2.91 | ... | 4.59 |
| Sr | ... | -1.90 | 1.00 | 1.07 |
| Y | ... | -1.80+-0.14 | 1.10+-0.14 | 0.44+-0.14 |
| Ba | ... | -0.87+-0.15 | 2.03+-0.15 | 1.26+-0.15 |
| La | ... | -0.78+-0.25 | 2.12+-0.25 | 0.39+-0.25 |
| Ce | ... | -0.95+-0.07 | 1.95+-0.07 | 0.63+-0.07 |
| Pr | ... | -1.25 | 1.65 | -0.54 |
| Nd | ... | -0.81+-0.21 | 2.09+-0.21 | 0.69+-0.21 |
| Eu | ... | -0.65 | 2.25 | -0.14 |
| Dy | ... | -1.40 | 1.50 | -0.26 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0034
| Title | New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34: Binarity and neutron capture elements |
| ADS | B.Barbuy et al.,AAP, 429, 1031, 2005 |
| Authors | B. Barbuy, M. Spite, F. Spite, V. Hill, R. Cayrel, B. Plez, P. Petitjean |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2452994 | HARPSESO | 100000 | 50,100 | 180min | -52.7+-0.3 |
| 2449975 | EMMIESO | 30000 | N/A | 120min | -44.6+-1.5 |
| 2449975 | EMMIESO | 30000 | N/A | 95min | -44.7+-1.5 |
| 2450025 | EMMIESO | 30000 | N/A | 90min | -46.6+-1.5 |
| 2450026 | EMMIESO | 30000 | N/A | 75min | -45.7+-1.5 |
| 2450358 | CASPECESO | 21000 | N/A | 120min | -43.3+-3.0 |
| 2450359 | CASPECESO | 21000 | N/A | 120min | -42.2+-3.0 |
| 2451575 | FEROSESO | 48000 | N/A | 30min | -44.2+-1.0 |
| 2451384 | FEROSESO | 48000 | N/A | 30min | -44.5+-1.0 |
| 2451394 | FEROSESO | 48000 | N/A | 30min | -44.7+-1.0 |
| 2452472 | VLT | 45000 | N/A | 45min | -51.4+-0.5 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 4800 |
| log g | 1.8 |
| vturb | 1.5 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| CH | ... | -0.28 | +2.63 | 8.24 |
| CN | ... | -0.53 | +2.38 | 7.39 |
| Na I | ... | -1.72+-0.19 | +1.18+-0.19 | 4.61+-0.19 |
| Mg I | ... | -2.18+-0.34 | +0.72+-0.34 | 5.40+-0.34 |
| Al I | ... | -2.91 | -0.01 | 3.56 |
| Ca I | ... | -2.45+-0.18 | +0.45+-0.18 | 3.91+-0.18 |
| Ti I | ... | -2.61+-0.28 | +0.29+-0.28 | 2.41+-0.28 |
| Ti II | ... | -2.46+-0.27 | +0.44+-0.27 | 2.56+-0.27 |
| Cr I | ... | -3.13+-0.12 | -0.23+-0.12 | 2.54+-0.12 |
| Fe I | ... | -2.90 | ... | 4.60 |
| Fe II | ... | -2.91 | ... | 4.59 |
| Ni I | ... | -2.89 | +0.01 | 3.36 |
| Zn I | ... | -2.44 | +0.46 | 2.15 |
| Sr II | ... | -1.90 | +1.00 | 1.02 |
| Y II | ... | -1.80 | +1.10 | 0.54 |
| Ba II | ... | -0.87 | +2.03 | 1.26 |
| La II | ... | -0.78 | +2.12 | 0.39 |
| Ce II | ... | -0.95 | +1.95 | 0.63 |
| Pr II | ... | -1.08 | +1.82 | -0.37 |
| Nd II | ... | -0.81 | +2.09 | 0.69 |
| Eu II | ... | -1.10 | +1.80 | -0.59 |
| Dy II | ... | -1.40 | +1.50 | -0.26 |
| Pb I | ... | +0.05 | +2.95 | 2.00 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0095
| Title | Bright Metal-poor Stars from the Hamburg/ESO Survey. I. Selection and Follow-up Observations from 329 Fields |
| ADS | A.Frebel et al.,ApJ, 652, 1585, 2006 |
| Authors | A. Frebel, N. Christlieb, J. E. Norris, T. C. Beers, M. S. Bessell, J. Rhee, C. Fechner, B. Marsteller, S. Rossi, C. Thom, L. Wisotzki, D. Reimers |
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Basic Informations
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -261853 |
| Right Ascension | 004139.7 |
Photometric data
| B | 13.4 |
| B-V | 0.79 |
| EB-V | 0.01 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -1.28 | 2.32 | 7.27 |
| Fe | ... | -3.60 | ... | 3.90 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0122
| Title | Carbon-enhanced Metal-poor Stars. I. Chemical Compositions of 26 Stars |
| ADS | W.Aoki et al.,ApJ, 655, 492, 2007 |
| Authors | W. Aoki, T. Beers, N. Christlieb, J. E. Norris, S. G. Ryan, S. Tsangarides |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2002-10-26 | N/A | SUBARUHDS | 50000 | N/A | 1200 | -49.52+-0.10 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -261853 |
| Right Ascension | 004139.7 |
Photometric data
| V | 12.221 |
| B | 13.338 |
| H | 10.115 |
| J | 10.571 |
| K | 9.996 |
| EB-V | 0.05 |
Atmospheric data
| Teff | 4900 |
| log g | 1.5 |
| vturb | 2.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -0.19+-0.20 | 2.72+-0.20 | 8.2+-0.20 |
| N | ... | -0.28+-0.53 | 2.63+-0.53 | 7.5+-0.53 |
| Na | ... | -1.13+-0.12 | 1.78+-0.12 | 5.03+-0.12 |
| Mg | ... | -1.60+-0.12 | 1.31+-0.12 | 5.93+-0.12 |
| Ca | ... | -2.39+-0.12 | 0.52+-0.12 | 3.91+-0.12 |
| Ti I | ... | -2.39+-0.11 | 0.52+-0.11 | 2.51+-0.11 |
| Ti II | ... | -2.50+-0.21 | 0.41+-0.21 | 2.40+-0.21 |
| Cr | ... | -3.06+-0.10 | -0.15+-0.10 | 2.57+-0.10 |
| Fe I | ... | -2.91+-0.27 | ... | 4.54+-0.27 |
| Fe II | ... | -2.89+-0.14 | ... | 4.56+-0.14 |
| Ba | ... | -0.68+-0.13 | 2.23+-0.13 | 1.49+-0.13 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio