BPS CS30325-094: found in 6 paper(s).
Labels:
/R.Cayrel et al.(2004)/
/M.Spite et al.(2005)/
/W.Aoki et al.(2005)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/S.M.Andrievsky et al.(2008)/
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A0016
Title | First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy |
ADS | R.Cayrel et al.,AAP, 416, 1117, 2004 |
Authors | R. Cayrel, E. Depagne, M. Spite, V. Hill, F. Spite, P. Francois, B. Plez, T. Beers, F. Primas, J. Andersen, B. Barbuy, P. Bonifacio, P. Molaro, B. Nordstrom |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07 | N/A | VLT | 47000 | 110 | 7200 | N/A |
2000-08 | N/A | VLT | 47000 | N/A | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
V | 12.33 |
B-V | 0.70 |
J-K | 0.48 |
V-K | 2.15 |
EB-V | 0.02 |
Atmospheric data
Teff | 4950 |
log g | 2.0 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -3.32 | -0.02 | 5.20 |
O I | ... | -2.58 | 0.72 | 6.19 |
Na I | ... | -3.21 | 0.09 | 3.12 |
Mg I | ... | -2.92+-0.14 | 0.38+-0.14 | 4.66+-0.14 |
Al I | ... | -3.88 | -0.58 | 2.59 |
Si I | ... | -2.49 | 0.81 | 5.06 |
K I | ... | -2.57 | 0.73 | 2.55 |
Ca I | ... | -2.92+-0.11 | 0.38+-0.11 | 3.44+-0.11 |
Sc II | ... | -2.97+-0.09 | 0.33+-0.09 | 0.20+-0.09 |
Ti I | ... | -3.03+-0.05 | 0.27+-0.05 | 1.99+-0.05 |
Ti II | ... | -3.01+-0.10 | 0.29+-0.10 | 2.01+-0.10 |
Cr I | ... | -3.74+-0.09 | -0.44+-0.09 | 1.93+-0.09 |
Mn I | ... | -3.85+-0.05 | -0.55+-0.05 | 1.54+-0.05 |
Fe I | ... | -3.30+-0.14 | 0.00+-0.14 | 4.20+-0.14 |
Fe II | ... | -3.30+-0.13 | 0.01+-0.13 | 4.20+-0.13 |
Co I | ... | -3.01+-0.08 | 0.29+-0.08 | 1.91+-0.08 |
Ni I | ... | -3.22+-0.04 | 0.08+-0.04 | 3.03+-0.04 |
Zn I | ... | -3.06 | 0.24 | 1.54 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0025
Title | First stars VI – Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements |
ADS | M.Spite et al.,AAP, 430, 655, 2005 |
Authors | M. Spite, R. Cayrel, B. Plez, V. Hill, F. Spite, E. Depagne, P. Francois, P. Bonifacio, B. Barbuy, T. Beers, J. Andersen, P. Molaro, B. Nordstrom, F. Primas |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | VLT | 47000 | 30 | 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 | 4950 |
log g | 2.0 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-1.41 | <1.89 | <-0.25 |
C | ... | -3.30+-0.05 | 0.00+-0.05 | 5.25+-0.05 |
N | ... | -3.12 | 0.18 | 4.85 |
O I | ... | -2.58 | 0.72 | 6.29 |
Fe | ... | -3.30 | ... | 4.20 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0057
Title | Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements |
ADS | W.Aoki et al.,ApJ, 632, 611, 2005 |
Authors | W. Aoki, S. Honda, T. C. Beers, T. Kajino, H. Ando, J. E. Norris, S. G. Ryan, H. Izumiura, K. Sadakane, M. Takada-Hidai |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-14 | N/A | SUBARUHDS | 50000 | 139 | 20min | -157.64+-0.25 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | +042138 |
Right Ascension | 145439.3 |
Binarity
Photometric data
V | 12.317 |
B | 13.019 |
H | 10.234 |
J | 10.682 |
K | 10.130 |
EB-V | 0.04 |
Atmospheric data
Teff | 5050 |
log g | 2.1 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -2.67 | 0.5 | 5.7 |
Mg I | ... | -2.62+-0.11 | 0.55+-0.11 | 4.96+-0.11 |
Al I | ... | -3.83+-0.18 | -0.66+-0.18 | 2.66+-0.18 |
Si I | ... | -2.31+-0.13 | 0.86+-0.13 | 5.25+-0.13 |
Ca I | ... | -2.83+-0.11 | 0.34+-0.11 | 3.52+-0.11 |
Sc II | ... | -2.80+-0.23 | 0.37+-0.23 | 0.3+-0.23 |
Ti I | ... | -2.77+-0.12 | 0.4+-0.12 | 2.17+-0.12 |
Ti II | ... | -2.73+-0.24 | 0.44+-0.24 | 2.21+-0.24 |
Cr I | ... | -3.63+-0.1 | -0.46+-0.1 | 2.06+-0.1 |
Mn I | ... | -4.22+-0.11 | -1.05+-0.11 | 1.31+-0.11 |
Fe I | ... | -3.17+-0.2 | ... | 4.33+-0.2 |
Fe II | ... | -3.14+-0.19 | ... | 4.36+-0.19 |
Co I | ... | -2.65+-0.11 | 0.52+-0.11 | 2.26+-0.11 |
Ni I | ... | -3.28+-0.11 | -0.11+-0.11 | 2.97+-0.11 |
Zn I | ... | -2.77+-0.21 | 0.4+-0.21 | 1.9+-0.21 |
Sr II | ... | -5.52+-0.24 | -2.35+-0.24 | -2.6+-0.24 |
Y II | ... | <-3.05 | <0.12 | <-0.82 |
Zr II | ... | <-3.04 | <0.13 | <-0.43 |
Ba II | ... | <-4.93 | <-1.76 | <-2.71 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0091
Title | First stars IX - Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios |
ADS | M.Spite et al.,AAP, 455, 291, 2006 |
Authors | M. Spite, R. Cayrel, V. Hill, F. Spite, P. Francois, B. Plez, P. Bonifacio, P. Molaro, E. Depagne, J. Andersen, B. Barbuy, T. C. Beers, B. Nordstrom, F. Primas |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 47000 | 130 | 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 | 4950 |
log g | 2.0 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.28+-0.05 | 0.02+-0.05 | 5.27+-0.05 |
N | ... | -3.12+-0.18 | 0.18+-0.18 | 4.85+-0.18 |
Fe | ... | -3.30 | ... | 4.20 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
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 | 4950 |
log g | 2.0 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na | ... | -3.41 | -0.11 | 2.84 |
Fe | ... | -3.30 | ... | 4.20 |
: 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 | 4950 |
log g | 2.0 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Al | ... | -3.22 | 0.08 | 3.25 |
Fe | ... | -3.30 | ... | 4.20 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)