BPS CS22965-054: 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 |
2001-06-04 | 2452064.3216247 | VLT | 43000 | 150 | 3600 | -281.6 |
2001-09-05 | 2452157.1919815 | VLT | 43000 | 150 | 2704 | -281.4 |
2001-09-05 | 2452157.2249206 | VLT | 43000 | 150 | 2700 | -281.6 |
2001-09-09 | 2452161.0744927 | VLT | 43000 | 150 | 5400 | -281.6 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | -023239 |
Right Ascension | 220630.0 |
Photometric data
Atmospheric data
Teff | 6089 |
log g | 3.75 |
vturb | 1.4 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 0.87+-0.09 | 3.91+-0.09 | 2.03+-0.09 |
Fe I | ... | -3.04 | ... | 4.46 |
: 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 | 6090 |
log g | 3.8 |
vturb | 1.4 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na | ... | -3.15 | -0.11 | 3.10 |
Fe | ... | -3.04 | ... | 4.46 |
: 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 |
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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 | 6090 |
log g | 3.8 |
vturb | 1.4 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Al | ... | -3.07 | -0.03 | 3.40 |
Fe | ... | -3.04 | ... | 4.46 |
: 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 |
2001-08-25 | N/A | KECKHIRES | N/A | 61 | 7200 | -283.0+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 6205+-100 |
log g | 3.73+-0.2 |
vturb | 1.7+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | <-2.02 | <1.07 | <6.53 |
Mg | ... | -2.78+-0.11 | 0.31+-0.11 | 4.80+-0.11 |
Al | ... | -3.82+-0.16 | -0.73+-0.16 | 2.65+-0.16 |
Si | ... | -3.01+-0.21 | 0.08+-0.21 | 4.54+-0.21 |
Ca | ... | -2.66+-0.07 | 0.43+-0.07 | 3.70+-0.07 |
Sc II | ... | -3.06+-0.18 | 0.03+-0.18 | 0.11+-0.18 |
Ti II | ... | -2.67+-0.07 | 0.42+-0.07 | 2.35+-0.07 |
Cr I | ... | -3.14+-0.07 | -0.05+-0.07 | 2.53+-0.07 |
Mn I | ... | -3.39+-0.12 | -0.30+-0.12 | 2.00+-0.12 |
Fe I | ... | -3.09+-0.03 | ... | 4.41+-0.03 |
Fe II | ... | -3.05+-0.14 | ... | 4.45+-0.14 |
Co | ... | -2.83+-0.16 | 0.26+-0.16 | 2.09+-0.16 |
Ni | ... | -3.09+-0.07 | 0.00+-0.07 | 3.16+-0.07 |
Sr II | ... | -3.03+-0.11 | 0.06+-0.11 | -0.06+-0.11 |
Ba II | ... | <-3.57 | <-0.48 | <-1.44 |
Eu II | ... | <-1.95 | <1.14 | <-1.44 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)