G4-36
taken from 3 paper(s):
/I.I.Ivans et al.(2003)/
/I.U.Roederer et al.(2014)/
/K.A.Venn et al.(2004)/
Chemical Substructure in the Milky Way Halo: A New Population of Old Stars
Stellar Parameters
Teff : 5975 | log g : 4.05 | vturb : 1.15 |
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 | ... | ... | 2.35 | -0.91 | 1.00 | 2.35 | Li I |
O I | 3 | ... | +0.30+-0.07 | ... | -1.39+-0.07 | 0.52+-0.07 | 7.30+-0.07 | O I |
Na I | 4 | ... | -0.28+-0.08 | ... | -2.12+-0.08 | -0.21+-0.08 | 4.12+-0.08 | Na I |
Mg I | 10 | ... | -0.19+-0.14 | ... | -2.14+-0.14 | -0.23+-0.14 | 5.46+-0.14 | Mg I |
Al I | 1 | ... | -1.44 | ... | -3.35 | -1.44 | 3.10 | Al I |
Si I | 1 | ... | -0.26 | ... | -2.15 | -0.24 | 5.36 | Si I |
K I | N/A | ... | <+0.15 | ... | <-1.69 | <0.22 | <3.34 | K I |
Ca I | 21 | ... | -0.21+-0.11 | ... | -2.12+-0.11 | -0.21+-0.11 | 4.22+-0.11 | Ca I |
Ca II | 1 | ... | -0.11 | ... | -2.02 | -0.11 | 4.32 | Ca II |
Sc II | 2 | ... | -0.76+-0.02 | ... | -2.75+-0.02 | -0.84+-0.02 | 0.40+-0.02 | Sc II |
Ti I | 13 | ... | +0.48+-0.08 | ... | -1.41+-0.08 | 0.50+-0.08 | 3.54+-0.08 | Ti I |
Ti II | 25 | ... | +0.60+-0.13 | ... | -1.29+-0.13 | 0.62+-0.13 | 3.66+-0.13 | Ti II |
V I | 2 | ... | +0.32+-0.03 | ... | -1.54+-0.03 | 0.37+-0.03 | 2.39+-0.03 | V I |
V II | 1 | ... | +0.55 | ... | -1.31 | 0.60 | 2.62 | V II |
Cr I | 13 | ... | +0.34+-0.08 | ... | -1.56+-0.08 | 0.35+-0.08 | 4.08+-0.08 | Cr I |
Cr II | 6 | ... | +0.48+-0.10 | ... | -1.42+-0.10 | 0.49+-0.10 | 4.22+-0.10 | Cr II |
Mn I | 10 | ... | +0.37+-0.09 | ... | -1.60+-0.09 | 0.31+-0.09 | 3.83+-0.09 | Mn I |
Fe I | 160 | -1.93+-0.11 | ... | ... | -1.91+-0.11 | ... | 5.59+-0.11 | Fe I |
Fe II | 20 | -1.95+-0.11 | ... | ... | -1.93+-0.11 | ... | 5.57+-0.11 | Fe II |
Co I | 3 | ... | +0.33+-0.20 | ... | -1.67+-0.20 | 0.24+-0.20 | 3.32+-0.20 | Co I |
Ni I | 24 | ... | +0.48+-0.11 | ... | -1.42+-0.11 | 0.49+-0.11 | 4.80+-0.11 | Ni I |
Cu I | N/A | ... | <-0.76 | ... | <-2.67 | <-0.76 | <1.52 | Cu I |
Zn I | 2 | ... | +1.00+-0.05 | ... | -0.89+-0.05 | 1.02+-0.05 | 3.67+-0.05 | Zn I |
Ga I | 1 | ... | +0.58+-0.10 | ... | -1.30+-0.10 | 0.61+-0.10 | 1.78+-0.10 | Ga I |
Sr II | 2 | ... | -0.65+-0.26 | ... | -2.55+-0.26 | -0.64+-0.26 | 0.32+-0.26 | Sr II |
Y II | N/A | ... | <-0.77 | ... | <-2.67 | <-0.76 | <-0.46 | Y II |
Ba II | 4 | ... | -0.72+-0.13 | ... | -2.70+-0.13 | -0.79+-0.13 | -0.52+-0.13 | Ba II |
La II | N/A | ... | <+1.38 | ... | <-0.43 | <1.48 | <0.67 | La II |
Eu II | N/A | ... | <+0.41 | ... | <-1.53 | <0.38 | <-1.01 | Eu II |
Position
Right Ascension : 02 43 22.05 | Declination : +13 25 57.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1996-11-05 | N/A | MCDONALD | 60000 | | 3600 | N/A |
1999-01-20 | N/A | MCDONALD | 60000 | 55-170 | 16200 | N/A |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 5810+-40 | log g : 3.65+-0.17 | 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 | 0.89 | 1.98 | Li I |
CH | 1 | ... | 0.30+-0.25 | 6.52 | -1.91 | 0.26+-0.25 | 6.52 | CH |
CN | 1 | ... | <1.83 | <7.45 | <-0.38 | <1.79 | <7.45 | CN |
O I | 1 | ... | 0.17+-0.20 | 6.69 | -2.00 | 0.17+-0.20 | 6.69 | O I |
Mg I | 7 | ... | -0.12+-0.23 | 5.32 | -2.28 | -0.11+-0.23 | 5.32 | Mg I |
Al I | 1 | ... | -1.42+-0.29 | 2.86 | -3.59 | -1.42+-0.29 | 2.86 | Al I |
Ca I | 10 | ... | -0.19+-0.22 | 3.98 | -2.36 | -0.19+-0.22 | 3.98 | Ca I |
Sc II | 3 | ... | -0.88+-0.16 | 0.05 | -3.10 | -0.93+-0.16 | 0.05 | Sc II |
Ti I | 15 | ... | 0.49+-0.20 | 3.28 | -1.67 | 0.50+-0.20 | 3.28 | Ti I |
Ti II | 19 | ... | 0.59+-0.14 | 3.32 | -1.63 | 0.54+-0.14 | 3.32 | Ti II |
V I | 1 | ... | 0.17+-0.22 | 1.93 | -2.00 | 0.17+-0.22 | 1.93 | V I |
V II | 2 | ... | 0.34+-0.24 | 2.05 | -1.88 | 0.29+-0.24 | 2.05 | V II |
Cr I | 9 | ... | 0.31+-0.20 | 3.78 | -1.86 | 0.31+-0.20 | 3.78 | Cr I |
Cr II | 3 | ... | 0.64+-0.14 | 4.06 | -1.58 | 0.59+-0.14 | 4.06 | Cr II |
Mn I | 8 | ... | 0.45+-0.22 | 3.72 | -1.71 | 0.46+-0.22 | 3.72 | Mn I |
Fe I | 87 | -2.17+-0.21 | ... | 5.33 | -2.17+-0.21 | ... | 5.33 | Fe I |
Fe II | 10 | -2.22+-0.14 | ... | 5.28 | -2.22+-0.14 | ... | 5.28 | Fe II |
Co I | 2 | ... | -0.27+-0.23 | 2.55 | -2.44 | -0.27+-0.23 | 2.55 | Co I |
Ni I | 8 | ... | 0.57+-0.22 | 4.62 | -1.60 | 0.57+-0.22 | 4.62 | Ni I |
Cu I | 1 | ... | <-0.04 | <1.98 | <-2.21 | <-0.04 | <1.98 | Cu I |
Zn I | 3 | ... | 1.13+-0.20 | 3.52 | -1.04 | 1.13+-0.20 | 3.52 | Zn I |
Sr II | 2 | ... | -1.32+-0.15 | -0.68 | -3.55 | -1.38+-0.15 | -0.68 | Sr II |
Y II | 1 | ... | -1.30+-0.36 | -1.31 | -3.52 | -1.35+-0.36 | -1.31 | Y II |
Mo I | 1 | ... | <1.22 | <0.93 | <-0.95 | <1.22 | <0.93 | Mo I |
Tc I | 1 | ... | ... | <1.10 | <1.10 | <3.27 | <1.10 | Tc I |
Sn I | 1 | ... | <2.13 | <2.03 | <-0.04 | <2.13 | <2.03 | Sn I |
Ba II | 1 | ... | -1.02+-0.14 | -1.06 | -3.24 | -1.07+-0.14 | -1.06 | Ba II |
Ce II | 4 | ... | <0.24 | <-0.40 | <-1.98 | <0.19 | <-0.40 | Ce II |
Pr II | 1 | ... | <1.35 | <-0.15 | <-0.87 | <1.30 | <-0.15 | Pr II |
Sm II | 2 | ... | <0.93 | <-0.33 | <-1.29 | <0.88 | <-0.33 | Sm II |
Eu II | 1 | ... | <0.38 | <-1.32 | <-1.84 | <0.33 | <-1.32 | Eu II |
Gd II | 2 | ... | <1.30 | <0.15 | <-0.92 | <1.25 | <0.15 | Gd II |
Tb II | 3 | ... | <1.25 | <-0.67 | <-0.99 | <1.18 | <-0.67 | Tb II |
Dy II | 1 | ... | <0.34 | <-0.78 | <-1.88 | <0.29 | <-0.78 | Dy II |
Er II | 3 | ... | <0.95 | <-0.35 | <-1.27 | <0.90 | <-0.35 | Er II |
Tm II | 2 | ... | <1.09 | <-1.03 | <-1.15 | <1.02 | <-1.03 | Tm II |
Yb II | 1 | ... | <-0.30 | <-1.60 | <-2.52 | <-0.35 | <-1.60 | Yb II |
Hf II | 2 | ... | <1.56 | <0.19 | <-0.52 | <1.65 | <0.19 | Hf II |
Ir I | 1 | ... | <2.10 | <1.31 | <-0.07 | <2.10 | <1.31 | Ir I |
Pb I | 1 | ... | <1.58 | <1.45 | <-0.59 | <1.58 | <1.45 | Pb I |
Binary Parameters
Binarity | Negative |
Vrad | 221.8 |
Position
Right Ascension : 02 43 22.05 | Declination : +13 25 57.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-10-30-07:15 | 2454769.808 | MCDONALD | 33000 | 50-130 | 7200 | 222.3 |
2008-11-01-07:58 | 2454771.838 | MCDONALD | 33000 | 50-130 | 5400 | 221.5 |
2008-11-04-06:45 | 2454774.787 | MCDONALD | 33000 | 50-130 | 7200 | 221.6 |
Stellar Chemical Signatures and Hierarchical Galaxy Formation
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 |
Na | N/A | ... | -0.28 | ... | -2.12 | -0.19 | 4.12 | Na |
Mg | N/A | ... | -0.19 | ... | -2.14 | -0.21 | 5.46 | Mg |
Ca | N/A | ... | -0.21 | ... | -2.12 | -0.19 | 4.22 | Ca |
Ti | N/A | ... | 0.54 | ... | -1.32 | 0.61 | 3.63 | Ti |
Fe | N/A | -1.93 | ... | ... | -1.93 | ... | 5.57 | Fe |
Ni | N/A | ... | 0.48 | ... | -1.42 | 0.51 | 4.80 | Ni |
Ba | N/A | ... | -0.72 | ... | -2.70 | -0.77 | -0.52 | Ba |
Position
Right Ascension : 02 43 22.05 | Declination : +13 25 57.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log