BD+03_740: found in 15 paper(s).
Labels:
/E.Carretta et al.(2002)/
/J.G.Cohen et al.(2002)/
/J.G.Cohen et al.(2004)/
/G.Israelian et al.(2001)/
/E.Arnone et al.(2005)/
/M.Asplund et al.(2006)/
/J.R.Shi et al.(2007)/
/A.M.Boesgaard and M. C. Novicki(2005)/
/J.P.Fulbright(2000)/
/G.Bihain et al.(2004)/
/A.Hosford et al.(2009)/
/L.Mashonkina et al.(2008)/
/D.K.Lai et al.(2008)/
/I.I.Ivans et al.(2003)/
/C.Charbonnel and F. Primas(2005)/
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A0028
Title | STELLAR ARCHAEOLOGY: A KECK PILOT PROGRAM ON EXTREMELY METAL-POOR STARS FROM THE HAMBURG/ESO SURVEY. II. ABUNDANCE ANALYSIS |
ADS | E.Carretta et al.,AJ, 124, 481, 2002 |
Authors | E. Carretta, R. Gratton, J. G. Palomar O. Cohen, T. C. Department of Physics and Astronomy, MSU. Beers, N. Christlieb |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-09 | N/A | KECKHIRES | 45000 | N/A | N/A | |
Photometric data
Atmospheric data
Teff | 6355 |
log g | 4.00 |
vturb | 1.42 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -2.34+-0.16 | 0.35+-0.16 | 5.24+-0.16 |
Al I | ... | -3.33+-0.10 | -0.64+-0.10 | 3.14+-0.10 |
Ca I | ... | -2.16+-0.05 | 0.53+-0.05 | 4.20+-0.05 |
Sc II | ... | -2.42+-0.07 | 0.27+-0.07 | 0.75+-0.07 |
Ti I | ... | -2.08+-0.04 | 0.61+-0.04 | 2.94+-0.04 |
Ti II | ... | -2.30+-0.06 | 0.39+-0.06 | 2.72+-0.06 |
Cr I | ... | -2.79+-0.08 | -0.10+-0.08 | 2.88+-0.08 |
Mn I | ... | -3.17+-0.06 | -0.48+-0.06 | 2.22+-0.06 |
Fe I | ... | -2.69+-0.11 | ... | 4.81+-0.11 |
Fe II | ... | -2.63+-0.14 | ... | 4.87+-0.14 |
Sr II | ... | -2.97+-0.02 | -0.28+-0.02 | 0.00+-0.02 |
Ba II | ... | -3.40 | -0.71 | -1.27 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0029
Title | STELLAR ARCHAEOLOGY: A KECK PILOT PROGRAM ON EXTREMELY METAL-POOR STARS FROM THE HAMBURG/ESO SURVEY. I. STELLAR PARAMETERS |
ADS | J.G.Cohen et al.,AJ, 124, 470, 2002 |
Authors | J. G. Palomar O. Cohen, N. Christlieb, T. C. Department of Physics and Astronomy, MSU. Beers, R. Gratton, E. Carretta |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-09 | N/A | KECKHIRES | 45000 | 240 | 240 | |
Binarity
Photometric data
V | 9.808 |
B-V | 0.36 |
U-B | -0.20 |
J | 8.77 |
K | 8.49 |
EB-V | 0.037 |
Atmospheric data
A0036
Title | Abundances In Very Metal-Poor Dwarf Stars |
ADS | J.G.Cohen et al.,ApJ, 612, 1107, 2004 |
Authors | J. G. Cohen, N. Christlieb, A. McWilliam, S. Shectman, I. Thompson, G. J. Wasserburg, I. Ivans, M. Dehn, T. Karlsson, J. Melendez |
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Basic Informations
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 6355 |
log g | 4.0 |
vturb | 1.4 |
A0046
Title | Oxygen in the Very Early Galaxy |
ADS | G.Israelian et al.,ApJ, 551, 833, 2001 |
Authors | G. Israelian, R. Rebolo, R. J. GarciaLopez, P. Bonifacio, P. Molaro, G. Basri, N. Shchukina |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1996-10-25 | N/A | WHTUES | 50000 | 220 | 3600 | 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 |
O I | ... | -1.94+-0.13 | 0.99 | 6.93+-0.13 |
Fe | ... | -2.93+-0.12 | ... | 4.57+-0.12 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0075
Title | Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing |
ADS | E.Arnone et al.,AAP, 430, 507, 2005 |
Authors | E. Arnone, S. G. Ryan, D. Argast, J. E. Norris, T. C. Beers |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | ANGLO | 40000 | >100 | 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 | 6240 |
log g | 3.7+-0.2 |
vturb | 1.8 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -2.52+-0.03 | 0.32+-0.03 | 5.06+-0.03 |
Ca I | ... | -2.43+-0.01 | 0.41+-0.01 | 3.93+-0.01 |
Fe I | ... | -2.84+-0.01 | ... | 4.66+-0.01 |
Fe II | ... | -2.87+-0.09 | ... | 4.63+-0.09 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0089
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-05-0103 | N/A | VLT | 120000 | 740 | 60 | 174.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
Atmospheric data
Teff | 6266 |
log g | 4.04 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li | ... | 0.96+-0.01 | 3.61+-0.01 | 2.12+-0.01 |
O | ... | -2.06 | 0.59 | 6.81 |
Fe | ... | -2.65 | ... | 4.85 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
A0113
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | FOCES | 40000 | 100-400 | N/A | N/A |
Photometric data
Atmospheric data
Teff | 6240 |
log g | 4.14 |
vturb | 1.60 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 0.99+-0.05 | 3.44+-0.05 | 2.15+-0.05 |
Fe | ... | -2.45 | ... | 5.05 |
: 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 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Be II | ... | -2.52 | 0.29 | -1.37 |
Fe | ... | -2.81 | ... | 4.69 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0126
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-10-30 | N/A | LICKHAMILTON | N/A | 100 | 3600 | |
Photometric data
Atmospheric data
Teff | 6075 |
log g | 3.8 |
vturb | 0.3 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 0.89 | 3.73 | 2.05 |
Na I | ... | -3.04 | -0.2 | 3.29 |
Mg I | ... | -2.26 | 0.58 | 5.32 |
Ca I | ... | -2.37 | 0.47 | 3.99 |
Cr I | ... | -5.67 | -2.83 | 0.00 |
Fe | ... | -2.84 | ... | 4.66 |
Ba II | ... | -3.34 | -0.5 | -1.21 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0136
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | WHTUES | N/A | 80-150 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 6229+-67 |
log g | 4.15+-0.27 |
vturb | 1.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.82 | ... | 4.68 |
Cu I | ... | <-3.77 | <-0.95 | <0.44 |
Zn I | ... | <-2.02 | <0.80 | <2.58 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0169
Title | Lithium abundances of halo dwarfs based on excitation temperature. I. Local thermodynamic equilibrium |
ADS | A.Hosford et al.,AAP, 493, 601, 2009 |
Authors | A. Hosford, S. G. Ryan, A. E. GarciaPerez, J. E. Norris, K. A. Olive |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ANGLO | 43000 | 100 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | 040224 |
Right Ascension | 045838 |
Photometric data
Atmospheric data
Teff | 6344+-113 |
log g | 4.44+-0.14 |
vturb | 1.50 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 1.02+-0.074 | 3.74+-0.074 | 2.18+-0.074 |
Fe | ... | -2.72 | ... | 4.78 |
Fe I | ... | -2.77 | ... | 4.73 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0179
Title | Non-LTE line formation for heavy elements in four very metal-poor stars |
ADS | L.Mashonkina et al.,ApJ, 679, 1549, 2008 |
Authors | L. Mashonkina, G. Zhao, T. Gehren, W. Aoki, M. Bergemann, K. Noguchi, J. R. Shi, M. Takada-Hidai, H. W. Zhang |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-02 | N/A | SUBARUHDS | 90000 | >100 | N/A | N/A |
| N/A | FOCES | 35000 | >100 | N/A | N/A |
| N/A | VLT | 48000 | >200 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 6340 |
log g | 3.90+-0.15 |
vturb | 1.4 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na | ... | -3.03+-0.02 | -0.38+-0.02 | 3.30+-0.02 |
Mg | ... | -2.40+-0.05 | 0.25+-0.05 | 5.18+-0.05 |
K | ... | -2.17+-0.04 | 0.48+-0.04 | 2.95+-0.04 |
Ca I | ... | -2.32+-0.07 | 0.33+-0.07 | 4.04+-0.07 |
Fe | ... | -2.65+-0.01 | ... | 4.85+-0.01 |
Sr | ... | -2.89 | -0.24 | 0.08 |
Ba | ... | -3.32 | -0.67 | -1.19 |
: 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 |
2004107-8 | N/A | KECKHIRES | N/A | 340 | 3900 | 173.1+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 6557+-100 |
log g | 4.28+-0.2 |
vturb | 1.8+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -2.12+-0.31 | 0.59+-0.31 | 6.43+-0.31 |
N | ... | <-2.42 | <0.29 | <5.55 |
OH | ... | <-1.73 | <0.98 | <7.14 |
Mg | ... | -2.48+-0.02 | 0.23+-0.02 | 5.10+-0.02 |
Al | ... | -3.55+-0.15 | -0.84+-0.15 | 2.92+-0.15 |
Si | ... | -2.64+-0.15 | 0.07+-0.15 | 4.91+-0.15 |
Ca | ... | -2.33+-0.03 | 0.38+-0.03 | 4.03+-0.03 |
Sc II | ... | -2.42+-0.05 | 0.29+-0.05 | 0.75+-0.05 |
Ti I | ... | -2.02+-0.03 | 0.69+-0.03 | 3.00+-0.03 |
Ti II | ... | -2.14+-0.06 | 0.57+-0.06 | 2.88+-0.06 |
V II | ... | -2.43+-0.09 | 0.28+-0.09 | 1.57+-0.09 |
Cr I | ... | -2.78+-0.03 | -0.07+-0.03 | 2.89+-0.03 |
Cr II | ... | -2.66+-0.09 | 0.05+-0.09 | 3.01+-0.09 |
Mn I | ... | -3.17+-0.09 | -0.46+-0.09 | 2.22+-0.09 |
Mn II | ... | -2.90+-0.06 | -0.19+-0.06 | 2.49+-0.06 |
Fe I | ... | -2.71+-0.08 | ... | 4.79+-0.08 |
Fe II | ... | -2.69+-0.06 | ... | 4.81+-0.06 |
Co | ... | -2.30+-0.05 | 0.41+-0.05 | 2.62+-0.05 |
Ni | ... | -2.65+-0.05 | 0.06+-0.05 | 3.60+-0.05 |
Cu | ... | -3.51+-0.06 | -0.80+-0.06 | 0.70+-0.06 |
Sr II | ... | -2.92+-0.09 | -0.21+-0.09 | 0.05+-0.09 |
Y II | ... | -2.72+-0.16 | -0.01+-0.16 | -0.48+-0.16 |
Zr II | ... | -2.35+-0.10 | 0.36+-0.10 | 0.25+-0.10 |
Ba II | ... | -3.08+-0.17 | -0.37+-0.17 | -0.95+-0.17 |
Eu II | ... | <-2.03 | <0.68 | <-1.52 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0188
Title | Chemical Substructure in the Milky Way Halo: A New Population of Old Stars |
ADS | I.I.Ivans et al.,ApJ, 592, 906, 2003 |
Authors | I. I. Ivans, C. Sneden, C. R. James, G. W. Preston, J. P. Fulbright, P. A. Hoflich, B. W. Carney, J. C. Wheeler |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-11-09 | N/A | MAYALLKPNO | 28000 | 100-150 | 1200 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | +040637 |
Right Ascension | 050116.6 |
Photometric data
V | 9.82 |
B-V | 0.36 |
EB-V | 0.07 |
Atmospheric data
Teff | 6330 |
log g | 3.55 |
vturb | 1.40 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <1.42 | <4.18 | <2.58 |
O I | ... | <-2.10 | <+0.66 | <6.77 |
Na I | ... | -3.02+-0.00 | -0.26+-0.00 | 3.31+-0.00 |
Mg I | ... | -2.36+-0.20 | +0.40+-0.20 | 5.22+-0.20 |
Ca I | ... | -2.39+-0.09 | +0.37+-0.09 | 3.97+-0.09 |
Sc II | ... | -2.45 | +0.31 | 0.72 |
Ti I | ... | -2.00+-0.15 | +0.76+-0.15 | 3.02+-0.15 |
Ti II | ... | -2.21+-0.09 | +0.55+-0.09 | 2.81+-0.09 |
V I | ... | <-0.16 | <+2.60 | <3.84 |
Cr I | ... | -2.68+-0.20 | +0.08+-0.20 | 2.99+-0.20 |
Mn I | ... | -2.38 | +0.38 | 3.01 |
Fe I | ... | -2.76+-0.12 | ... | 4.74+-0.12 |
Fe II | ... | -2.74+-0.07 | ... | 4.76+-0.07 |
Ni I | ... | -2.34+-0.35 | +0.42+-0.35 | 3.91+-0.35 |
Cu I | ... | <-1.36 | <+1.40 | <2.85 |
Y II | ... | <-1.93 | <+0.83 | <0.31 |
Ba II | ... | <-2.60 | <+0.16 | <-0.47 |
Eu II | ... | <-0.13 | <+2.63 | <0.38 |
: 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 | 4.11028 |
Right Ascension | 75.31926 |
Photometric data
V | 9.81 |
B-V | 0.36 |
EB-V | 0.049 |
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | 0.99+-0.026 | 3.76+-0.026 | 2.155+-0.026 |
Fe | ... | -2.77+-0.080 | ... | 4.73+-0.080 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)