G206-34
taken from 4 paper(s):
/C.Charbonnel and F. Primas(2005)/
/J.A.Rich and A. M. Boesgaard(2009)/
/I.U.Roederer et al.(2014)/
/A.M.Boesgaard et al.(2011)/
The lithium content of the Galactic Halo stars
Stellar Parameters
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 |
Li I | N/A | ... | ... | 2.208+0.045-0.054 | -1.05+0.045-0.054 | 1.91+0.045-0.054 | 2.208+0.045-0.054 | Li I |
Fe | N/A | -2.96+-0.100 | ... | ... | -2.96+-0.100 | ... | 4.54+-0.100 | Fe |
Position
Right Ascension : 18 35 19.17 | Declination : +28 41 55.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
BERYLLIUM, OXYGEN, AND IRON ABUNDANCES IN EXTREMELY METAL-DEFICIENT STARS
Stellar Parameters
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 |
Be II | N/A | ... | ... | -1.2+-0.11 | -2.58+-0.11 | 0.54+-0.11 | -1.2+-0.11 | Be II |
OH | N/A | -2.37+-0.14 | ... | ... | -2.19+-0.14 | 0.93+-0.14 | 6.50+-0.14 | OH |
Fe | N/A | -3.12+-0.09 | ... | ... | -3.12+-0.09 | ... | 4.38+-0.09 | Fe |
Position
Right Ascension : 18 35 19.17 | Declination : +28 41 55.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-05-15 | N/A | KECKHIRES | 48000 | 97 | 6300 | N/A |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 5930+-38 | log g : 3.6+-0.16 | vturb : 1.35+-0.06 |
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 |
Li I | 1 | ... | ... | 1.98 | -1.28 | 1.89 | 1.98 | Li I |
CH | 1 | ... | 0.54+-0.25 | 5.84 | -2.59 | 0.58+-0.25 | 5.84 | CH |
CN | 1 | ... | <3.40 | <8.10 | <0.27 | <3.44 | <8.10 | CN |
Mg I | 7 | ... | 0.39+-0.22 | 4.83 | -2.77 | 0.40+-0.22 | 4.83 | Mg I |
Al I | 2 | ... | -0.71+-0.22 | 2.57 | -3.88 | -0.71+-0.22 | 2.57 | Al I |
Si I | 1 | ... | 0.45+-0.36 | 4.79 | -2.72 | 0.45+-0.36 | 4.79 | Si I |
Ca I | 10 | ... | 0.46+-0.23 | 3.63 | -2.71 | 0.46+-0.23 | 3.63 | Ca I |
Sc II | 1 | ... | -0.17+-0.14 | -0.15 | -3.30 | -0.13+-0.14 | -0.15 | Sc II |
Ti I | 5 | ... | 0.43+-0.23 | 2.21 | -2.74 | 0.43+-0.23 | 2.21 | Ti I |
Ti II | 13 | ... | 0.15+-0.15 | 1.97 | -2.98 | 0.19+-0.15 | 1.97 | Ti II |
Cr I | 3 | ... | -0.21+-0.20 | 2.26 | -3.38 | -0.21+-0.20 | 2.26 | Cr I |
Mn I | 4 | ... | -0.32+-0.22 | 1.94 | -3.49 | -0.32+-0.22 | 1.94 | Mn I |
Fe I | 68 | -3.17+-0.21 | ... | 4.33 | -3.17+-0.21 | ... | 4.33 | Fe I |
Fe II | 4 | -3.13+-0.16 | ... | 4.37 | -3.13+-0.16 | ... | 4.37 | Fe II |
Co I | 2 | ... | 0.01+-0.27 | 1.83 | -3.16 | 0.01+-0.27 | 1.83 | Co I |
Ni I | 3 | ... | -0.05+-0.24 | 3.00 | -3.22 | -0.05+-0.24 | 3.00 | Ni I |
Zn I | 2 | ... | 0.50+-0.27 | 1.89 | -2.67 | 0.50+-0.27 | 1.89 | Zn I |
Rb I | 1 | ... | <2.96 | <2.31 | <-0.05 | <3.12 | <2.31 | Rb I |
Sr II | 2 | ... | -0.07+-0.17 | -0.33 | -3.20 | -0.03+-0.17 | -0.33 | Sr II |
Y II | 3 | ... | <0.00 | <-0.92 | <-3.13 | <0.04 | <-0.92 | Y II |
Zr II | 3 | ... | <0.42 | <-0.13 | <-2.71 | <0.46 | <-0.13 | Zr II |
Nb II | 1 | ... | <2.94 | <1.27 | <-0.19 | <2.98 | <1.27 | Nb II |
Mo I | 1 | ... | <2.12 | <0.83 | <-1.05 | <2.12 | <0.83 | Mo I |
Tc I | 1 | ... | ... | <1.04 | <1.04 | <4.21 | <1.04 | Tc I |
Ba II | 2 | ... | -0.07+-0.15 | -1.01 | -3.19 | -0.02+-0.15 | -1.01 | Ba II |
Ce II | 5 | ... | <1.24 | <-0.31 | <-1.89 | <1.28 | <-0.31 | Ce II |
Pr II | 5 | ... | <1.74 | <-0.67 | <-1.39 | <1.78 | <-0.67 | Pr II |
Nd II | 4 | ... | <1.39 | <-0.32 | <-1.74 | <1.43 | <-0.32 | Nd II |
Sm II | 2 | ... | <1.65 | <-0.52 | <-1.48 | <1.69 | <-0.52 | Sm II |
Eu II | 4 | ... | <1.08 | <-1.53 | <-2.05 | <1.12 | <-1.53 | Eu II |
Gd II | 3 | ... | <1.91 | <-0.15 | <-1.22 | <1.95 | <-0.15 | Gd II |
Tb II | 4 | ... | <2.22 | <-0.61 | <-0.93 | <2.24 | <-0.61 | Tb II |
Dy II | 2 | ... | <1.38 | <-0.65 | <-1.75 | <1.42 | <-0.65 | Dy II |
Ho II | 2 | ... | <1.89 | <-0.76 | <-1.23 | <1.94 | <-0.76 | Ho II |
Er II | 3 | ... | <1.85 | <-0.36 | <-1.28 | <1.89 | <-0.36 | Er II |
Tm II | 2 | ... | <2.20 | <-0.83 | <-0.95 | <2.22 | <-0.83 | Tm II |
Yb II | 1 | ... | <1.17 | <-1.04 | <-1.96 | <1.21 | <-1.04 | Yb II |
Hf II | 2 | ... | <2.59 | <0.31 | <-0.40 | <2.77 | <0.31 | Hf II |
Ir I | 1 | ... | <3.09 | <1.30 | <-0.08 | <3.09 | <1.30 | Ir I |
Pb I | 1 | ... | <2.28 | <1.15 | <-0.89 | <2.28 | <1.15 | Pb I |
Th II | 2 | ... | <2.38 | <-0.69 | <-0.75 | <2.42 | <-0.69 | Th II |
Binary Parameters
Binarity | Positive |
Vrad | -85.9 |
Position
Right Ascension : 18 35 19.17 | Declination : +28 41 55.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-09-06-02:57 | 2454715.625 | MCDONALD | 33000 | 50-135 | 7200 | -80.4 |
2008-09-07-03:12 | 2454716.635 | MCDONALD | 33000 | 50-135 | 7200 | -78.2 |
2009-06-11-09:46 | 2454993.91 | MCDONALD | 33000 | 50-135 | 8000 | -91.8 |
Beryllium and Alpha-element Abundances in a Large Sample of Metal-poor Stars
Stellar Parameters
Teff : 5825+-100 | log g : 3.99+-0.2 | vturb : 1.5+-0.2 |
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 |
Be | N/A | ... | +0.50+-0.15 | -1.20+-0.12 | -2.58+-0.12 | 0.54+-0.15 | -1.20+-0.12 | Be |
O | N/A | -2.37+-0.22 | +0.75+-0.24 | ... | -2.43+-0.22 | 0.69+-0.24 | 6.26+-0.22 | O |
Mg | N/A | -2.55+-0.07 | ... | ... | -2.57+-0.07 | 0.55+-0.07 | 5.03+-0.07 | Mg |
Ti | N/A | -2.65+-0.09 | ... | ... | -2.58+-0.09 | 0.54+-0.09 | 2.37+-0.09 | Ti |
Fe | N/A | -3.12+-0.09 | ... | ... | -3.12+-0.09 | ... | 4.38+-0.09 | Fe |
Position
Right Ascension : | Declination : | 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 | KECKHIRES | 42000 | N/A | N/A | N/A |