HD115444: found in 12 paper(s).
Labels:
/D.L.Burris et al.(2000)/
/S.Honda et al.(2004)/
/J.A.Johnson(2002)/
/J.Westin et al.(2000)/
/W.Aoki et al.(2003)/
/J.J.Cowan et al.(2005)/
/S.Honda et al.(2004)/
/D.K.Lai et al.(2007)/
/J.Simmerer et al.(2004)/
/C.Sneden et al.(1998)/
/J.A.Johnson and M. Bolte(2002)/
/J.A.Johnson and M. Bolte(2001)/
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A0014
Title | NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS |
ADS | D.L.Burris et al.,ApJ, 544, 302, 2000 |
Authors | D. L. Burris, C. A. Pilachowski, T. E. Armandroff, C. Sneden, J. J. Cowan, H. Roe |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MAYALLKPNO | 20000 | 100-200 | 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 | 4750 |
log g | 1.70 |
vturb | 1.60 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.77 | ... | 4.73 |
Ba | ... | -2.82 | -0.05 | -0.69 |
Eu | ... | -2.12 | 0.65 | -1.61 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0017
Title | Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium |
ADS | S.Honda et al.,ApJ, 607, 474, 2004 |
Authors | S. Honda, W. Aoki, T. Kajino, H. Ando, T. C. Beers, H. Izumiura, K. Sadakane, M. Takada-Hidai |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07-04 | N/A | SUBARUHDS | 90000 | 255 | 3900 | -27.30+-0.34 |
2001-01-28 | N/A | SUBARUHDS | N/A | N/A | N/A | -27.58+-0.25 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 8.97 |
B | 9.75 |
B-V | 0.78 |
V-K | 2.36 |
H | 6.70 |
J | 7.16 |
K | 6.61 |
EB-V | 0.00 |
Atmospheric data
Teff | 4720 |
log g | 1.5 |
vturb | 1.7 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -3.26 | -0.41 | 5.3 |
Mg I | ... | -2.46+-0.03 | 0.39+-0.03 | 5.12+-0.03 |
Al I | ... | -3.33+-0.11 | -0.48+-0.11 | 3.14+-0.11 |
Si I | ... | -2.50+-0.11 | 0.35+-0.11 | 5.05+-0.11 |
Ca I | ... | -2.58+-0.06 | 0.27+-0.06 | 3.78+-0.06 |
Sc II | ... | -2.87 | -0.02 | 0.3 |
Ti | ... | -2.55+-0.1 | 0.3+-0.1 | 2.47+-0.1 |
V | ... | -2.90+-0.15 | -0.05+-0.15 | 1.1+-0.15 |
Cr | ... | -2.79+-0.17 | 0.06+-0.17 | 2.88+-0.17 |
Mn I | ... | -3.38+-0.12 | -0.53+-0.12 | 2.01+-0.12 |
Fe | ... | -2.85+-0.15 | ... | 4.66+-0.15 |
Co I | ... | -2.66+-0.12 | 0.19+-0.12 | 2.26+-0.12 |
Ni I | ... | -2.96+-0.11 | -0.11+-0.11 | 3.29+-0.11 |
Sr II | ... | -2.81+-0.11 | 0.04+-0.11 | 0.11+-0.11 |
Y II | ... | -3.01+-0.08 | -0.16+-0.08 | -0.78+-0.08 |
Zr II | ... | -2.67+-0.17 | 0.18+-0.17 | -0.06+-0.17 |
Pd I | ... | -2.76+-0.11 | 0.09+-0.11 | -1.06+-0.11 |
Ba II | ... | -2.71+-0.11 | 0.14+-0.11 | -0.49+-0.11 |
La II | ... | -2.75+-0.05 | 0.1+-0.05 | -1.53+-0.05 |
Ce II | ... | -2.73+-0.1 | 0.12+-0.1 | -1.1+-0.1 |
Pr II | ... | -2.29+-0.11 | 0.56+-0.11 | -1.49+-0.11 |
Nd II | ... | -2.55+-0.06 | 0.3+-0.06 | -1.06+-0.06 |
Sm II | ... | -2.22+-0.19 | 0.63+-0.19 | -1.24+-0.19 |
Eu II | ... | -2.19+-0.03 | 0.66+-0.03 | -1.64+-0.03 |
Gd II | ... | -2.19+-0.21 | 0.66+-0.21 | -1.1+-0.21 |
Tb II | ... | -2.64+-0.11 | 0.21+-0.11 | -2.29+-0.11 |
Dy II | ... | -2.24+-0.09 | 0.61+-0.09 | -1.07+-0.09 |
Er II | ... | -2.23+-0.09 | 0.62+-0.09 | -1.26+-0.09 |
Tm II | ... | -2.33+-0.11 | 0.52+-0.11 | -2.18+-0.11 |
Yb II | ... | -2.42+-0.11 | 0.43+-0.11 | -1.46+-0.11 |
Ir I | ... | -2.26+-0.11 | 0.59+-0.11 | -0.89+-0.11 |
Th II | ... | -2.06+-0.15 | 0.79+-0.15 | -1.97+-0.15 |
U II | ... | <-1.85 | <1.00 | <-2.35 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
A0031
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-05-12 | N/A | KECKHIRES | 45000 | 400 | 2400 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | N/A | 1200 | N/A |
1999-03-08 | N/A | LICKHAMILTON | 60000 | 90 | 3600 | N/A |
1997-05-12 | N/A | KECKHIRES | 45000 | 400 | 2400 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | N/A | 1200 | N/A |
1999-03-08 | N/A | LICKHAMILTON | 60000 | 90 | 3600 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 9.00 |
V-R | 0.746 |
V-K | 2.327 |
EB-V | 0.00 |
Atmospheric data
Teff | 4500 |
log g | 0.70 |
vturb | 2.25 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -2.76+-0.10 | 0.37+-0.10 | 3.57+-0.10 |
Mg I | ... | -2.32+-0.10 | 0.81+-0.10 | 5.26+-0.10 |
Al I | ... | -3.23+-0.10 | -0.10+-0.10 | 3.24+-0.10 |
Si I | ... | -2.55+-0.20 | 0.58+-0.20 | 5.00+-0.20 |
Ca I | ... | -2.73+-0.06 | 0.40+-0.06 | 3.63+-0.06 |
Sc II | ... | -3.15+-0.09 | -0.02+-0.09 | 0.02+-0.09 |
Ti I | ... | -2.86+-0.09 | 0.27+-0.09 | 2.16+-0.09 |
Ti II | ... | -2.87+-0.08 | 0.26+-0.08 | 2.15+-0.08 |
V I | ... | -3.21+-0.03 | -0.08+-0.03 | 0.79+-0.03 |
V II | ... | -2.99+-0.08 | 0.14+-0.08 | 1.01+-0.08 |
Cr I | ... | -3.32+-0.08 | -0.19+-0.08 | 2.35+-0.08 |
Cr II | ... | -2.90+-0.05 | 0.23+-0.05 | 2.77+-0.05 |
Mn I | ... | -3.47+-0.02 | -0.34+-0.02 | 1.92+-0.02 |
Mn II | ... | -3.22+-0.07 | -0.09+-0.07 | 2.17+-0.07 |
Fe I | ... | -3.13+-0.13 | ... | 4.37+-0.13 |
Fe II | ... | -3.14+-0.08 | ... | 4.36+-0.08 |
Co I | ... | -2.79+-0.13 | 0.34+-0.13 | 2.13+-0.13 |
Ni I | ... | -3.01+-0.18 | 0.12+-0.18 | 3.24+-0.18 |
Zn I | ... | -2.88+-0.04 | 0.25+-0.04 | 1.72+-0.04 |
Y II | ... | -3.24+-0.10 | -0.11+-0.10 | -1.00+-0.10 |
Zr II | ... | -2.90+-0.13 | 0.23+-0.13 | -0.30+-0.13 |
Ba II | ... | -3.23+-0.08 | -0.10+-0.08 | -1.10+-0.08 |
La II | ... | -2.85+-0.05 | 0.28+-0.05 | -1.68+-0.05 |
Ce II | ... | -3.11+-0.11 | 0.02+-0.11 | -1.53+-0.11 |
Pr II | ... | -2.86+-0.20 | 0.27+-0.20 | -2.15+-0.20 |
Nd II | ... | -2.86+-0.20 | 0.27+-0.20 | -1.36+-0.20 |
Sm II | ... | -2.60+-0.09 | 0.53+-0.09 | -1.59+-0.09 |
Eu II | ... | -2.33+-0.03 | 0.80+-0.03 | -1.82+-0.03 |
Gd II | ... | -2.59+-0.20 | 0.54+-0.20 | -1.47+-0.20 |
Tb II | ... | -2.31+-0.15 | 0.82+-0.15 | -2.41+-0.15 |
Dy II | ... | -2.44+-0.13 | 0.69+-0.13 | -1.30+-0.13 |
Er II | ... | -2.33+-0.04 | 0.80+-0.04 | -1.40+-0.04 |
Tm II | ... | -2.36+-0.15 | 0.77+-0.15 | -2.36+-0.15 |
Yb II | ... | -2.36+-0.20 | 0.77+-0.20 | -1.28+-0.20 |
Os I | ... | <-2.25 | <0.88 | <-0.80 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0033
Title | THE r-PROCESS-ENRICHED LOW-METALLICITY GIANT HD 115444 |
ADS | J.Westin et al.,ApJ, 530, 783, 2000 |
Authors | J. Westin, C. Sneden, B. Gustafsson, J. J. Department of Physics and Astronomy, UofOklahoma. Cowan |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 200,400,500 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 8.96 |
B-V | 0.75 |
U-B | 0.16 |
V-K | 2.34 |
Atmospheric data
Teff | 4650 |
log g | 1.50 |
vturb | 2.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O I | ... | -2.32+-0.11 | +0.66+-0.11 | +6.60+-0.11 |
Na I | ... | -2.98+-0.11 | 0.00+-0.11 | +3.34+-0.11 |
Mg I | ... | -2.44+-0.12 | +0.54+-0.12 | +5.13+-0.12 |
Al I | ... | -3.34+-0.11 | -0.36+-0.11 | +3.12+-0.11 |
Si I | ... | -2.52+-0.11 | +0.46+-0.11 | +5.02+-0.11 |
Ca I | ... | -2.60+-0.06 | +0.38+-0.06 | +3.75+-0.06 |
Sc II | ... | -2.81+-0.05 | +0.17+-0.05 | +0.28+-0.05 |
Ti I | ... | -2.58+-0.06 | +0.40+-0.06 | +2.40+-0.06 |
Ti II | ... | -2.53+-0.13 | +0.45+-0.13 | +2.45+-0.13 |
V I | ... | -2.85+-0.20 | +0.13+-0.20 | +1.14+-0.20 |
V II | ... | -2.83+-0.11 | +0.15+-0.11 | +1.16+-0.11 |
Cr I | ... | -3.26+-0.13 | -0.28+-0.13 | +2.40+-0.13 |
Mn I | ... | -3.48+-0.16 | -0.50+-0.16 | +1.90+-0.16 |
Fe I | ... | -2.98+-0.10 | ... | +4.54+-0.10 |
Fe II | ... | -3.00+-0.07 | ... | +4.52+-0.07 |
Co I | ... | -2.67+-0.10 | +0.31+-0.10 | +2.24+-0.10 |
Ni I | ... | -2.99+-0.03 | -0.01+-0.03 | +3.25+-0.03 |
Cu I | ... | -3.67+-0.11 | -0.69+-0.11 | +0.53+-0.11 |
Zn I | ... | -2.73+-0.11 | +0.25+-0.11 | +1.86+-0.11 |
Ge I | ... | -3.45+-0.11 | -0.47+-0.11 | -0.05+-0.11 |
Sr II | ... | -2.66+-0.11 | +0.32+-0.11 | +0.23+-0.11 |
Y II | ... | -3.05+-0.12 | -0.07+-0.12 | -0.82+-0.12 |
Zr II | ... | -2.61+-0.12 | +0.37+-0.12 | -0.02+-0.12 |
Ba II | ... | -2.80+-0.09 | +0.18+-0.09 | -0.68+-0.09 |
La II | ... | -2.61+-0.10 | +0.37+-0.10 | -1.40+-0.10 |
Ce II | ... | -2.64+-0.12 | +0.34+-0.12 | -1.10+-0.12 |
Pr II | ... | -2.52+-0.34 | +0.46+-0.34 | -1.82+-0.34 |
Nd II | ... | -2.42+-0.12 | +0.56+-0.12 | -0.93+-0.12 |
Sm II | ... | -2.17+-0.16 | +0.81+-0.16 | -1.18+-0.16 |
Eu II | ... | -2.13+-0.07 | +0.85+-0.07 | -1.63+-0.07 |
Gd II | ... | -2.09+-0.13 | +0.89+-0.13 | -0.98+-0.13 |
Dy II | ... | -2.10+-0.10 | +0.88+-0.10 | -1.01+-0.10 |
Ho II | ... | -2.34+-0.11 | +0.64+-0.11 | -1.85+-0.11 |
Er II | ... | -2.13+-0.02 | +0.85+-0.02 | -1.21+-0.02 |
Tm II | ... | -1.91+-0.11 | +1.07+-0.11 | -1.79+-0.11 |
Yb II | ... | -2.47+-0.11 | +0.51+-0.11 | -1.40+-0.11 |
Os I | ... | -1.99+-0.11 | +0.99+-0.11 | -0.55+-0.11 |
Pt I | ... | -2.09+-0.11 | +0.89+-0.11 | -0.30+-0.11 |
Th II | ... | -2.34+-0.11 | +0.64+-0.11 | -2.23+-0.11 |
U II | ... | <-2.48 | <+0.5 | <-2.6 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
A0072
Title | Measurement of the Europium Isotope Ratio for the Extremely Metal poor, r-Process-enhanced Star CS 31082-001 |
ADS | W.Aoki et al.,ApJ, 586, 506, 2003 |
Authors | W. Aoki, S. Honda, T. C. Beers, C. Sneden |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07-05 | 2451730.8 | SUBARUHDS | 90000 | 300 | 2x30min | -27.12+-0.34 |
2001-04-16 | 2452016.0 | SUBARUHDS | 90000 | 300 | 2x30min | -27.11+-0.28 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Isotope ratio
A0076
Title | Hubble Space Telescope Observations of Heavy Elements in Metal-Poor Galactic Halo Stars |
ADS | J.J.Cowan et al.,ApJ, 627, 238, 2005 |
Authors | J. J. Cowan, C. Sneden, T. C. Beers, J. E. Lawler, J. Simmerer, J. W. Truran, F. Primas, J. Collier, S. Burles |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | HST | 30000 | >50 | N/A | N/A |
N/A | N/A | KECKHIRES | 45000 | 30-200 | N/A | |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4720 |
log g | 1.75 |
vturb | 2.00 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -2.90 | ... | 4.60 |
Fe II | ... | -2.71 | ... | 4.79 |
Ge | ... | -3.67 | -0.77 | -0.07 |
Zr | ... | -3.00 | -0.10 | -0.20 |
La | ... | -2.70 | +0.20 | -1.35 |
Eu | ... | -2.32 | +0.58 | -1.61 |
Os | ... | -2.06 | +0.84 | -0.65 |
Ir | ... | -2.04 | +0.86 | -0.68 |
Pt | ... | -2.18 | +0.72 | -0.48 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0085
Title | Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. I. Observational Data |
ADS | S.Honda et al.,ApJS, 152, 113, 2004 |
Authors | S. Honda, W. Aoki, H. Ando, H. Izumiura, T. Kajino, E. Kambe, S. Kawanomoto, K. Noguchi, K. Okita, K. Sadakane, B. Sato, M. Takada-Hidai, Y. Takeda, E. Watanabe, T. C. Beers, J. E. Norris, S. G. Ryan |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07-04 | N/A | SUBARUHDS | 90000 | 255 | 3900 | -27.30+-0.34 |
2001-01-28 | N/A | SUBARUHDS | N/A | N/A | N/A | -27.58+-0.25 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
A0128
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | KECKII | 7000 | N/A | N/A | N/A |
Atmospheric data
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.01+-0.19 | -0.15+-0.19 | 5.54+-0.19 |
Fe | ... | -2.86 | ... | 4.64 |
Sr | ... | -2.60 | 0.26 | 0.37 |
Ba | ... | -2.52 | 0.34 | -0.39 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0131
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Atmospheric data
Teff | 4721 |
log g | 1.74 |
vturb | 2.00 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.45 | -0.55 | 5.10 |
Fe I | ... | -2.90 | ... | 4.60 |
Fe II | ... | -2.71 | ... | 4.79 |
La II | ... | -2.52+-0.07 | 0.38+-0.07 | -1.35+-0.07 |
Eu II | ... | -2.12+-0.03 | 0.78+-0.03 | -1.61+-0.03 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0132
Title | Hubble Space Telescope Observations of Neutron-Capture Elements in Very Metal Poor Stars |
ADS | C.Sneden et al.,ApJ, 496, 235, 1998 |
Authors | C. Sneden, J. J. Cowan, D. L. Burris, J. W. Truran |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | 32000 | 50-70 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4750 |
log g | 1.70 |
vturb | 1.6 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Ge I | ... | -3.51 | -0.75 | -0.10 |
Zr II | ... | -2.45 | +0.25 | +0.15 |
Os I | ... | -2.00 | -0.75 | -0.55 |
Pt I | ... | -2.02 | -0.75 | -0.22 |
Pb I | ... | -2.35 | -0.30 | -0.4 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0185
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-05-12 | N/A | KECKHIRES | 45000 | 400 | 2400 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | N/A | 1200 | N/A |
1999-03-08 | N/A | LICKHAMILTON | 60000 | 90 | 3600 | N/A |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -3.14 | ... | 4.36 |
Sr II | ... | -3.48+-0.30 | -0.34+-0.30 | -0.51+-0.30 |
Y II | ... | -3.24+-0.09 | -0.10+-0.09 | -1.00+-0.09 |
Zr II | ... | -2.90+-0.08 | 0.24+-0.08 | -0.30+-0.08 |
Pd I | ... | <-2.18 | <0.96 | <-0.49 |
Ba II | ... | -3.23+-0.15 | -0.09+-0.15 | -1.10+-0.15 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0186
Get more information of this paper.
Atmospheric data
Teff | 4500 |
log g | 0.70 |
vturb | 2.25 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -3.15+-0.11 | ... | 4.35+-0.11 |
Fe II | ... | -3.16+-0.06 | ... | 4.34+-0.06 |
Ba II | ... | -3.22+-0.15 | -0.07+-0.15 | -1.09+-0.15 |
La II | ... | -2.89+-0.07 | 0.26+-0.07 | -1.72+-0.07 |
Ce II | ... | -3.07+-0.11 | 0.08+-0.11 | -1.49+-0.11 |
Pr II | ... | -2.85+-0.15 | 0.30+-0.15 | -2.14+-0.15 |
Nd II | ... | -2.85+-0.10 | 0.30+-0.10 | -1.35+-0.10 |
Sm II | ... | -2.58+-0.10 | 0.57+-0.10 | -1.57+-0.10 |
Eu II | ... | -2.32+-0.05 | 0.83+-0.05 | -1.81+-0.05 |
Gd II | ... | -2.58+-0.20 | 0.57+-0.20 | -1.46+-0.20 |
Tb II | ... | -2.73+-0.12 | 0.42+-0.12 | -2.83+-0.12 |
Dy II | ... | -2.39+-0.07 | 0.76+-0.07 | -1.25+-0.07 |
Er II | ... | -2.32+-0.04 | 0.83+-0.04 | -1.39+-0.04 |
Tm II | ... | -2.48+-0.11 | 0.67+-0.11 | -2.48+-0.11 |
Yb II | ... | -2.35+-0.28 | 0.80+-0.28 | -1.27+-0.28 |
Os I | ... | <-2.25 | <0.90 | <-0.80 |
Th II | ... | -2.48+-0.09 | 0.67+-0.09 | -2.48+-0.09 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio