BPS CS29506-007: found in 4 paper(s).
Labels:
/P.Bonifacio et al.(2007)/
/S.M.Andrievsky et al.(2007)/
/S.M.Andrievsky et al.(2008)/
/D.K.Lai et al.(2008)/
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A0109
| Title | First stars VII - Lithium in extremely metal poor dwarfs |
| ADS | P.Bonifacio et al.,AAP, 462, 851, 2007 |
| Authors | P. Bonifacio, P. Molaro, T. Sivarani, R. Cayrel, M. Spite, F. Spite, B. Plez, J. Andersen, B. Barbuy, T. C. Beers, E. Depagne, V. Hill, P. Francois, B. Nordstrom, F. Primas |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-09-06 | 2452158.0936928 | VLT | 43000 | 223 | 5400 | 56.4 |
| 2001-09-09 | 2452161.0276342 | VLT | 43000 | 223 | 3600 | 56.4 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -204624 |
| Right Ascension | 212028.6 |
Photometric data
Atmospheric data
| Teff | 6273 |
| log g | 4.00 |
| vturb | 1.7 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | 0.99+-0.09 | 3.90+-0.09 | 2.15+-0.09 |
| Fe I | ... | -2.91 | ... | 4.59 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0110
| Title | NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars |
| ADS | S.M.Andrievsky et al.,AAP, 464, 1081, 2007 |
| Authors | S. M. Andrievsky, M. Spite, S. A. Korotin, F. Spite, P. Bonifacio, R. Cayrel, V. Hill, P. Francois |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | VLT | 43000 | 200 | 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 | 6270 |
| log g | 4.0 |
| vturb | 1.7 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Na | ... | -3.10 | -0.19 | 3.15 |
| Fe | ... | -2.91 | ... | 4.59 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0176
| Title | NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars |
| ADS | S.M.Andrievsky et al.,AAP, 481, 481, 2008 |
| Authors | S. M. Andrievsky, M. Spite, S. A. Korotin, F. Spite, P. Bonifacio, R. Cayrel, V. Hill, P. François |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | VLT | 47000 | 120 | N/A | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Atmospheric data
| Teff | 6270 |
| log g | 4.0 |
| vturb | 1.7 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Al | ... | -2.99 | -0.08 | 3.48 |
| Fe | ... | -2.91 | ... | 4.59 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0181
| Title | Detailed Abundances for 28 Metal-poor Stars: Stellar Relics in the Milky Way |
| ADS | D.K.Lai et al.,ApJ, 681, 1524, 2008 |
| Authors | D. K. Lai, M. Bolte, J. A. Johnson, S. Lucatello |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2004-10-08 | N/A | KECKHIRES | N/A | 81 | 5400 | 55.1+-0.2 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6369+-100 |
| log g | 3.84+-0.2 |
| vturb | 1.4+-0.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | <-2.02 | <0.83 | <6.53 |
| N | ... | <-1.92 | <0.93 | <6.05 |
| OH | ... | <-1.33 | <1.52 | <7.54 |
| Mg | ... | -2.57+-0.05 | 0.28+-0.05 | 5.01+-0.05 |
| Al | ... | -3.67+-0.15 | -0.82+-0.15 | 2.80+-0.15 |
| Si | ... | -2.75+-0.15 | 0.10+-0.15 | 4.80+-0.15 |
| Ca | ... | -2.40+-0.05 | 0.45+-0.05 | 3.96+-0.05 |
| Sc II | ... | -2.57+-0.08 | 0.28+-0.08 | 0.60+-0.08 |
| Ti I | ... | -2.19+-0.06 | 0.66+-0.06 | 2.83+-0.06 |
| Ti II | ... | -2.28+-0.07 | 0.57+-0.07 | 2.74+-0.07 |
| Cr I | ... | -3.02+-0.04 | -0.17+-0.04 | 2.65+-0.04 |
| Mn I | ... | -3.54+-0.09 | -0.69+-0.09 | 1.85+-0.09 |
| Mn II | ... | -3.27+-0.16 | -0.42+-0.16 | 2.12+-0.16 |
| Fe I | ... | -2.85+-0.08 | ... | 4.65+-0.08 |
| Fe II | ... | -2.89+-0.07 | ... | 4.61+-0.07 |
| Co | ... | -2.57+-0.15 | 0.28+-0.15 | 2.35+-0.15 |
| Ni | ... | -2.91+-0.06 | -0.06+-0.06 | 3.34+-0.06 |
| Cu | ... | <-3.41 | <-0.56 | <0.80 |
| Sr II | ... | -2.72+-0.09 | 0.13+-0.09 | 0.25+-0.09 |
| Y II | ... | -2.61+-0.16 | 0.24+-0.16 | -0.37+-0.16 |
| Zr II | ... | -2.22+-0.10 | 0.63+-0.10 | 0.38+-0.10 |
| Ba II | ... | -2.74+-0.17 | 0.11+-0.17 | -0.61+-0.17 |
| Eu II | ... | <-1.97 | <0.88 | <-1.46 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)