BPS CS22949-037: found in 10 paper(s).
Labels:
/E.Depagne et al.(2002)/
/J.E.Norris et al.(2001)/
/R.Cayrel et al.(2004)/
/M.Spite et al.(2005)/
/J.E.Norris et al.(2002)/
/A.McWilliam et al.(1995)/
/A.McWilliam et al.(1995)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/J.G.Cohen et al.(2008)/
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A0005
Title | First Stars II. Elemental abundances in the extremely metal-poor star CS 22949–037 A diagnostic of early massive supernovae |
ADS | E.Depagne et al.,AAP, 390, 187, 2002 |
Authors | E. Depagne, V. Hill, M. Spite, F. Spite, B. Plez, T. C. Department of Physics and Astronomy, MSU. Beers, B. Barbuy, R. Cayrel, J. Andersen, P. Bonifacio, P. Francois, B. Nordstrom, F. Primas |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-08-08-0454 | N/A | VLT | 45000 | 110-170 | 1h | -125.68+-0.2 |
2000-08-08-0557 | N/A | VLT | 45000 | 110-170 | 1h | |
2000-08-09-0401 | N/A | VLT | 45000 | 110-170 | 1h | |
2000-08-09-0504 | N/A | VLT | 45000 | 110-170 | 1h | -125.64+-0.2 |
2000-08-11-0427 | N/A | VLT | 45000 | 110-170 | 1h | -125.60+-0.2 |
2000-08-11-0536 | N/A | VLT | 45000 | 110-170 | 1h | |
2001-09-06-0506 | N/A | VLT | 45000 | 40-90 | 1h | -125.62+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
V | 14.36 |
B-V | 0.730 |
V-R | 0.715 |
V-K | 2.298 |
Atmospheric data
Teff | 4900 |
log g | 1.5 |
vturb | 1.8 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.8 | 1.17 | 5.72 |
CN | ... | -1.4 | 2.57 | 6.52 |
O I | ... | -1.99 | 1.98 | 6.84 |
Na I | ... | -1.88+-0.03 | 2.09+-0.03 | 3.8+-0.03 |
Mg I | ... | -2.41+-0.19 | 1.58+-0.19 | 5.17+-0.19 |
Al I | ... | -4.13+-0.03 | -0.16+-0.03 | 2.34+-0.03 |
Si I | ... | -3.25 | 0.72 | 4.05 |
S I | ... | -2.12 | +1.78 | 5.09 |
K I | ... | -4.06 | -0.09 | 0.89 |
Ca I | ... | -3.63+-0.17 | 0.35+-0.17 | 2.73+-0.17 |
Sc II | ... | -3.87+-0.14 | 0.1+-0.14 | -0.7+-0.14 |
Ti I | ... | -3.62+-0.09 | 0.35+-0.09 | 1.4+-0.09 |
Ti II | ... | -3.61+-0.15 | 0.36+-0.15 | 1.41+-0.15 |
Cr I | ... | -4.38+-0.1 | -0.41+-0.1 | 1.29+-0.1 |
Mn I | ... | -4.78+-0.01 | -0.81+-0.01 | 0.61+-0.01 |
Fe I | ... | -3.99+-0.11 | ... | 3.51+-0.11 |
Fe II | ... | -3.94+-0.11 | ... | 3.56+-0.11 |
Co I | ... | -3.64+-0.07 | 0.33+-0.07 | 1.28+-0.07 |
Ni I | ... | -4.06+-0.02 | -0.07+-0.02 | 2.19+-0.02 |
Zn I | ... | -3.41 | 0.7 | 1.29 |
Sr II | ... | -3.64+-0.06 | 0.33+-0.06 | -0.72+-0.06 |
Y II | ... | -4.04+-0.11 | -0.07+-0.11 | -1.8+-0.11 |
Ba II | ... | -4.55+-0.1 | -0.58+-0.1 | -2.42+-0.1 |
Sm II | ... | -2.83 | +1.14 | -1.82 |
Eu II | ... | -3.93 | +0.04 | -3.42 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0012
Title | EXTREMELY METAL-POOR STARS. VIII. HIGH-RESOLUTION, HIGH SIGNAL-TO-NOISE RATIO ANALYSIS OF FIVE STARS WITH [Fe/H]<=-3.5 |
ADS | J.E.Norris et al.,ApJ, 561, 1034, 2001 |
Authors | J. E. Norris, S. G. Ryan, T. C. Beers |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-09-05 | N/A | ANGLO | 42000 | N/A | N/A | -125.7+-1.19 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
V | 14.36 |
B-V | 0.74 |
V-R | 0.49 |
Atmospheric data
Teff | 4900 |
log g | 1.7 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -2.74+-0.20 | 1.05+-0.20 | 5.81+-0.20 |
CN | ... | -1.09+-0.40 | 2.70+-0.40 | 6.88+-0.40 |
Mg I | ... | -2.57+-0.14 | 1.22+-0.14 | 5.01+-0.14 |
Al I | ... | -4.22+-0.32 | -0.43+-0.32 | 2.25+-0.32 |
Si I | ... | -2.75+-0.30 | 1.04+-0.30 | 4.80+-0.30 |
Ca I | ... | -3.34+-0.21 | 0.45+-0.21 | 3.02+-0.21 |
Sc II | ... | -3.66+-0.20 | 0.13+-0.20 | -0.49+-0.20 |
Ti I | ... | <-3.77+-0.04 | <0.02+-0.04 | <1.25+-0.04 |
Ti II | ... | -3.44+-0.16 | 0.35+-0.16 | 1.58+-0.16 |
V II | ... | <-3.14+-0.19 | <0.65+-0.19 | <0.86+-0.19 |
Cr I | ... | -4.34+-0.17 | -0.55+-0.17 | 1.33+-0.17 |
Mn I | ... | -4.71+-0.21 | -0.92+-0.21 | 0.68+-0.21 |
Fe I | ... | -3.79+-0.16 | ... | 3.71+-0.16 |
Fe II | ... | -3.79+-0.29 | ... | 3.71+-0.29 |
Co I | ... | -3.21+-0.21 | 0.58+-0.21 | 1.71+-0.21 |
Ni I | ... | -3.73+-0.15 | 0.06+-0.15 | 2.52+-0.15 |
Sr II | ... | -3.69+-0.23 | 0.10+-0.23 | -0.72+-0.23 |
Y II | ... | -3.60+-0.25 | 0.19+-0.25 | -1.36+-0.25 |
Ba II | ... | -4.63+-0.32 | -0.84+-0.32 | -2.50+-0.32 |
Eu II | ... | <-2.86+-0.18 | <0.93+-0.18 | <-2.35+-0.18 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
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 |
2000-08 | N/A | VLT | 47000 | 110 | 30000 | N/A |
2001-09 | N/A | VLT | N/A | 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 | 14.36 |
B-V | 0.72 |
V-R | 0.70 |
J-K | 0.52 |
V-K | 2.22 |
EB-V | 0.02 |
Atmospheric data
Teff | 4900 |
log g | 1.5 |
vturb | 1.8 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -2.80 | 1.17 | 5.72 |
CN | ... | -1.40 | 2.57 | 6.52 |
O I | ... | -1.99 | 1.98 | 6.78 |
Na I | ... | -2.53 | 1.44 | 3.80 |
Mg I | ... | -2.41+-0.19 | 1.56+-0.19 | 5.17+-0.19 |
Al I | ... | -4.13 | -0.17 | 2.34 |
Si I | ... | -3.20 | 0.77 | 4.35 |
K I | ... | -3.74 | 0.23 | 1.38 |
Ca I | ... | -3.63+-0.17 | 0.34+-0.17 | 2.73+-0.17 |
Sc II | ... | -3.87+-0.14 | 0.09+-0.14 | -0.70+-0.14 |
Ti I | ... | -3.62+-0.09 | 0.35+-0.09 | 1.40+-0.09 |
Ti II | ... | -3.61+-0.15 | 0.36+-0.15 | 1.41+-0.15 |
Cr I | ... | -4.38+-0.10 | -0.42+-0.10 | 1.29+-0.10 |
Mn I | ... | -4.43 | -0.47 | 0.96 |
Fe I | ... | -3.99+-0.11 | -0.03+-0.11 | 3.51+-0.11 |
Fe II | ... | -3.94+-0.11 | 0.02+-0.11 | 3.56+-0.11 |
Co I | ... | -3.64+-0.07 | 0.33+-0.07 | 1.28+-0.07 |
Ni I | ... | -4.06+-0.02 | -0.10+-0.02 | 2.19+-0.02 |
Zn I | ... | -3.31 | 0.66 | 1.29 |
: 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 | 4900 |
log g | 1.5 |
vturb | 1.8 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-1.46 | <2.51 | <-0.30 |
C | ... | -2.82+-0.10 | 1.15+-0.10 | 5.73+-0.10 |
N | ... | -1.82 | 2.15 | 6.15 |
O I | ... | -1.99 | 1.98 | 6.88 |
Fe | ... | -3.97 | ... | 3.53 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0030
Title | EXTREMELY METAL-POOR STARS. IX. CS 22949-037 AND THE ROLE OF HYPERNOVAE |
ADS | J.E.Norris et al.,ApJ, 569, L107, 2002 |
Authors | J. E. Research School of Astronomy and Astrophysics, Australian National University, MountStromloO. Norris, S. G. Department of Physics and Astronomy, OpenU. Ryan, T. C. Department of Physics and Astronomy, MSU. Beers, W. Aoki, H. Ando |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-08-24 | N/A | ANGLO | N/A | N/A | 300min | N/A |
2001-07-28 | N/A | SUBARUEEV | N/A | N/A | 165min | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.74 | 1.05 | 5.81 |
CN | ... | -1.49+-0.4 | 2.3+-0.4 | 6.48+-0.4 |
Fe | ... | -3.79 | ... | 3.71 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0038
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | FRUTTI | 22000 | N/A | N/A | N/A |
Photometric data
V | 14.35 |
B-V | 0.744 |
V-R | 0.492 |
A0039
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FRUTTI | 22000 | 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
V | 14.35 |
B-V | 0.744 |
V-R | 0.492 |
Atmospheric data
Teff | 4810 |
log g | 2.10+-0.45 |
vturb | 2.09+-0.17 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.11 | 0.88 | 5.44 |
Na | ... | -1.83 | 2.16 | 4.50 |
Mg | ... | -2.79 | 1.20 | 4.79 |
Ca | ... | -3.09 | 0.90 | 3.27 |
Fe I | ... | -3.99 | ... | 3.51 |
Fe II | ... | -3.99 | ... | 3.51 |
Sr | ... | -3.57 | 0.42 | -0.60 |
Ba | ... | -4.15 | -0.16 | -2.02 |
: 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 | 4900 |
log g | 1.5 |
vturb | 1.8 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.72+-0.10 | 1.25+-0.10 | 5.83+-0.10 |
N | ... | -1.72+-0.30 | 2.25+-0.30 | 6.25+-0.30 |
Fe | ... | -3.97 | ... | 3.53 |
: 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 | 4900 |
log g | 1.5 |
vturb | 1.8 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na | ... | -2.40 | +1.57 | 3.85 |
Fe | ... | -3.97 | ... | 3.53 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0187
Title | New Extremely Metal-Poor Stars in the Galactic Halo |
ADS | J.G.Cohen et al.,ApJ, 672, 320, 2008 |
Authors | J. G. Cohen, N. Christlieb, A. McWilliam, S. Shectman, I. Thompson, J. Melendez, L. Wisotzki, D. Reimers |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2451764.73 | | | | | -125.6+-0.1 |
| 2452158.73 | | | | | -125.6+-0.1 |
| 2452544.90 | KECKHIRES | 46000 | 100 | 7200 | -125.9+-0.1 |
| 2453312.76 | KECKHIRES | 46000 | 100 | 7200 | -125.9+-0.1 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | -023958 |
Right Ascension | 232629.8 |
Photometric data
Atmospheric data
Teff | 4915 |
log g | 1.70 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -2.82 | 0.97 | 5.77 |
NH | ... | -1.63+-0.30 | 2.16+-0.30 | 6.30+-0.30 |
OH | ... | -1.83 | 1.96 | 7.20 |
Na I | ... | -2.34+-0.11 | 1.45+-0.11 | 3.98+-0.11 |
Mg I | ... | -2.32+-0.25 | 1.47+-0.25 | 5.22+-0.25 |
Al I | ... | -3.31 | 0.48 | 3.16 |
Si I | ... | -3.23 | 0.56 | 4.32 |
Ca I | ... | -3.48+-0.11 | 0.31+-0.11 | 2.88+-0.11 |
Ca II | ... | -3.71 | 0.08 | 2.65 |
Sc II | ... | -3.67 | 0.12 | -0.56 |
Ti I | ... | <-3.33 | <0.46 | <1.66 |
Ti II | ... | -3.52+-0.06 | 0.27+-0.06 | 1.47+-0.06 |
V II | ... | -3.70+-0.03 | 0.09+-0.03 | 0.30+-0.03 |
Cr I | ... | -4.33+-0.15 | -0.54+-0.15 | 1.34+-0.15 |
Mn I | ... | -4.76+-0.03 | -0.97+-0.03 | 0.63+-0.03 |
Mn II | ... | -4.22+-0.01 | -0.43+-0.01 | 1.17+-0.01 |
Fe I | ... | -3.79+-0.16 | ... | 3.66+-0.16 |
Fe II | ... | -3.73+-0.18 | 0.06+-0.18 | 3.72+-0.18 |
Co I | ... | -3.37+-0.18 | 0.42+-0.18 | 1.55+-0.18 |
Ni I | ... | -4.05+-0.04 | -0.26+-0.04 | 2.20+-0.04 |
Cu I | ... | -4.57 | -0.78 | -0.36 |
Sr II | ... | -3.61+-0.02 | 0.18+-0.02 | -0.71+-0.02 |
Ba II | ... | -4.45+-0.23 | -0.66+-0.23 | -2.32+-0.23 |
Eu II | ... | <-3.06 | <0.73 | <-2.55 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)