BS16082-129
taken from 3 paper(s):
/S.Honda et al.(2004)/
/S.Honda et al.(2004)/
/D.M.Allen et al.(2012)/
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium
Stellar Parameters
Teff : 4900 | log g : 1.8 | vturb : 1.6 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
CH | N/A | ... | 0.29 | 5.99 | -2.44 | 0.41 | 5.99 | CH |
Mg I | 7 | ... | 0.28+-0.15 | 5+-0.15 | -2.60+-0.15 | 0.25+-0.15 | 5+-0.15 | Mg I |
Al I | 1 | ... | -0.94+-0.16 | 2.67+-0.16 | -3.78+-0.16 | -0.93+-0.16 | 2.67+-0.16 | Al I |
Si I | 1 | ... | 0.36+-0.16 | 5.05+-0.16 | -2.46+-0.16 | 0.39+-0.16 | 5.05+-0.16 | Si I |
Ca I | 4 | ... | 0.31+-0.04 | 3.81+-0.04 | -2.53+-0.04 | 0.32+-0.04 | 3.81+-0.04 | Ca I |
Sc II | 2 | ... | -0.01+-0.06 | 0.3+-0.06 | -2.85+-0.06 | -0.00+-0.06 | 0.3+-0.06 | Sc II |
Ti | 22 | ... | 0.24+-0.12 | 2.4+-0.12 | -2.55+-0.12 | 0.30+-0.12 | 2.4+-0.12 | Ti |
V | 2 | ... | 0.02+-0.16 | 1.16+-0.16 | -2.77+-0.16 | 0.08+-0.16 | 1.16+-0.16 | V |
Cr | 3 | ... | ... | 2.81+-0.16 | -2.83+-0.16 | 0.02+-0.16 | 2.81+-0.16 | Cr |
Mn I | 6 | ... | -0.31+-0.1 | 2.22+-0.1 | -3.21+-0.1 | -0.36+-0.1 | 2.22+-0.1 | Mn I |
Fe | 76 | -2.86+-0.15 | ... | 4.65+-0.15 | -2.85+-0.15 | ... | 4.65+-0.15 | Fe |
Co I | 3 | ... | 0.32+-0.13 | 2.38+-0.13 | -2.61+-0.13 | 0.24+-0.13 | 2.38+-0.13 | Co I |
Ni I | 2 | ... | -0.19+-0.16 | 3.2+-0.16 | -3.02+-0.16 | -0.17+-0.16 | 3.2+-0.16 | Ni I |
Sr II | 1 | ... | -0.73+-0.16 | -0.67+-0.16 | -3.54+-0.16 | -0.69+-0.16 | -0.67+-0.16 | Sr II |
Y II | 4 | ... | -0.56+-0.25 | -1.19+-0.25 | -3.40+-0.25 | -0.55+-0.25 | -1.19+-0.25 | Y II |
Zr II | 4 | ... | -0.01+-0.36 | -0.26+-0.36 | -2.84+-0.36 | 0.01+-0.36 | -0.26+-0.36 | Zr II |
Ba II | 2 | ... | -0.97+-0.16 | -1.61+-0.16 | -3.79+-0.16 | -0.94+-0.16 | -1.61+-0.16 | Ba II |
Isotopic Ratio
Position
Right Ascension : 13 47 11.50 | Declination : +28 57 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-01-30 | N/A | SUBARUHDS | 50000 | 55 | 5400 | -92.16+-0.30 |
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. I. Observational Data
Binary Parameters
Position
Right Ascension : 13 47 11.50 | Declination : +28 57 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-01-30 | N/A | SUBARUHDS | 50000 | 55 | 5400 | -92.16+-0.30 |
Elemental abundances and classification of carbon-enhanced metal-poor stars
Stellar Parameters
Teff : 5080+-50 | log g : 1.98+-0.11 | vturb : 1.30+-0.05 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | 1.20+-0.30 | 7.13 | -1.30 | 1.35+-0.30 | 7.13 | C |
Ti | N/A | ... | 0.59+-0.26 | 3.02 | -1.93 | 0.72+-0.26 | 3.02 | Ti |
Cr | N/A | ... | 0.59+-0.20 | 3.67 | -1.97 | 0.68+-0.20 | 3.67 | Cr |
Fe I | N/A | -2.65 | ... | ... | -2.65 | ... | 4.85 | Fe I |
Fe II | N/A | -2.59 | ... | ... | -2.59 | ... | 4.91 | Fe II |
Zn | N/A | ... | 0.59+-0.72 | 2.60 | -1.96 | 0.69+-0.72 | 2.60 | Zn |
Sr II | N/A | ... | -0.41+-0.30 | -0.03 | -2.90 | -0.25+-0.30 | -0.03 | Sr II |
Y | N/A | ... | 0.09+-0.26 | -0.26 | -2.47 | 0.18+-0.26 | -0.26 | Y |
Zr | N/A | ... | 0.59+-0.70 | 0.60 | -1.98 | 0.67+-0.70 | 0.60 | Zr |
Ba | N/A | ... | -0.41+-0.21 | -0.87 | -3.05 | -0.40+-0.21 | -0.87 | Ba |
Ce | N/A | ... | 0.67+-0.37 | -0.22 | -1.80 | 0.85+-0.37 | -0.22 | Ce |
Nd | N/A | ... | 0.64+-0.16 | -0.50 | -1.92 | 0.73+-0.16 | -0.50 | Nd |
Position
Right Ascension : 13 47 11.50 | Declination : +28 57 46.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | WHTUES | 52000 | 45 | N/A | N/A |