HD340279: found in 6 paper(s).
Labels:
/P.E.Nissen et al.(2007)/
/C.J.Akerman et al.(2004)/
/A.M.Boesgaard and M. C. Novicki(2005)/
/J.Melendez et al.(2006)/
/P.E.Nissen et al.(2004)/
/C.Charbonnel and F. Primas(2005)/
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A0119
| Title | Sulphur and zinc abundances in Galactic halo stars revisited |
| ADS | P.E.Nissen et al.,AAP, 469, 319, 2007 |
| Authors | P. E. Nissen, C. Ackerman, M. Asplund, D. Fabbian, F. Kerber, H. U. Kaufl, M. Pettini |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2007-06-25 | N/A | VLT | 60000 | N/A | N/A | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6417 |
| log g | 4.42 |
| vturb | 1.5 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| S I | ... | -2.35 | 0.19 | 4.98 |
| Fe | ... | -2.54 | ... | 4.96 |
| Zn I | ... | -2.35 | 0.19 | 2.25 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0123
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 60000 | 200-300 | 3600 | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Atmospheric data
| Teff | 6273 |
| log g | 4.25 |
| vturb | 1.5 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C I | ... | -2.41 | 0.21 | 6.14 |
| O I | ... | -2.16 | 0.46 | 6.71 |
| Fe | ... | -2.62 | ... | 4.88 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0124
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2003-03-27 | N/A | SUBARUHDS | 50000 | 98 | 6000 | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6200+-40 |
| log g | 4.48+-0.20 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Be II | ... | <-3.15+-0.09 | <-0.44+-0.09 | <-2.00+-0.09 |
| Fe | ... | -2.71+-0.12 | ... | 4.79+-0.12 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0143
| Title | PERMITTED OXYGEN ABUNDANCES AND THE TEMPERATURE SCALE OF METAL-POOR TURNOFF STARS |
| ADS | J.Melendez et al.,ApJ, 642, 1082, 2006 |
| Authors | J. Melendez, N. G. Shchukina, I. E. Vasiljeva, I. Ramirez |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 60000 | 200-300 | N/A | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6521+-102 |
| log g | 4.31+-0.15 |
| vturb | 1.5 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| O I | ... | -2.18 | 0.38 | 6.69 |
| Fe II | ... | -2.56 | ... | 4.94 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0160
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2001 | N/A | VLT | 60000 | 150-300 | N/A | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6273+-70 |
| log g | 4.25+-0.15 |
| vturb | 1.5+-0.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| S I | ... | -2.43 | 0.19 | 4.90 |
| Fe II | ... | -2.62 | ... | 4.88 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0191
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Basic Informations
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | 25.05197 |
| Right Ascension | 306.18922 |
Photometric data
| V | 10.828 |
| B-V | 0.427 |
| EB-V | 0.4 |
Atmospheric data
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | <-0.05 | <2.78 | <1.108 |
| Fe | ... | -2.83+-0.030 | ... | 4.67+-0.030 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)