G15-10
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Teff : 5050+-41 | log g : 4.05+-0.3 | vturb : 0.9+-0.12 |
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 | ... | ... | 0.60 | -2.66 | -0.13 | 0.60 | Li I |
CH | 1 | ... | 0.20+-0.25 | 6.09 | -2.34 | 0.19+-0.25 | 6.09 | CH |
NH | 1 | ... | -0.66+-0.36 | 4.63 | -3.20 | -0.67+-0.36 | 4.63 | NH |
O I | 1 | ... | 1.14+-0.13 | 7.30 | -1.39 | 1.14+-0.13 | 7.30 | O I |
Mg I | 5 | ... | 0.42+-0.12 | 5.49 | -2.11 | 0.42+-0.12 | 5.49 | Mg I |
Al I | 1 | ... | -0.45+-0.22 | 3.47 | -2.98 | -0.45+-0.22 | 3.47 | Al I |
Ca I | 10 | ... | 0.37+-0.14 | 4.18 | -2.16 | 0.37+-0.14 | 4.18 | Ca I |
Sc II | 4 | ... | -0.06+-0.14 | 0.55 | -2.60 | -0.07+-0.14 | 0.55 | Sc II |
Ti I | 18 | ... | 0.16+-0.09 | 2.58 | -2.37 | 0.16+-0.09 | 2.58 | Ti I |
Ti II | 24 | ... | 0.29+-0.14 | 2.70 | -2.25 | 0.28+-0.14 | 2.70 | Ti II |
V I | 1 | ... | -0.12+-0.13 | 1.28 | -2.65 | -0.12+-0.13 | 1.28 | V I |
Cr I | 10 | ... | -0.06+-0.09 | 3.05 | -2.59 | -0.06+-0.09 | 3.05 | Cr I |
Cr II | 2 | ... | 0.33+-0.17 | 3.43 | -2.21 | 0.32+-0.17 | 3.43 | Cr II |
Mn I | 4 | ... | -0.44+-0.09 | 2.46 | -2.97 | -0.44+-0.09 | 2.46 | Mn I |
Mn II | 3 | ... | -0.37+-0.20 | 2.52 | -2.91 | -0.38+-0.20 | 2.52 | Mn II |
Fe I | 104 | -2.53+-0.10 | ... | 4.97 | -2.53+-0.10 | ... | 4.97 | Fe I |
Fe II | 8 | -2.54+-0.15 | ... | 4.96 | -2.54+-0.15 | ... | 4.96 | Fe II |
Co I | 5 | ... | -0.20+-0.18 | 2.26 | -2.73 | -0.20+-0.18 | 2.26 | Co I |
Ni I | 12 | ... | 0.00+-0.16 | 3.69 | -2.53 | 0.00+-0.16 | 3.69 | Ni I |
Cu I | 1 | ... | <-0.53 | <1.13 | <-3.06 | <-0.53 | <1.13 | Cu I |
Zn I | 2 | ... | 0.18+-0.13 | 2.21 | -2.35 | 0.18+-0.13 | 2.21 | Zn I |
Rb I | 1 | ... | <1.97 | <1.96 | <-0.40 | <2.13 | <1.96 | Rb I |
Sr II | 2 | ... | -0.15+-0.09 | 0.17 | -2.70 | -0.17+-0.09 | 0.17 | Sr II |
Y II | 1 | ... | -0.29+-0.17 | -0.62 | -2.83 | -0.30+-0.17 | -0.62 | Y II |
Zr II | 3 | ... | 0.13+-0.15 | 0.17 | -2.41 | 0.12+-0.15 | 0.17 | Zr II |
Nb II | 1 | ... | <2.06 | <0.98 | <-0.48 | <2.05 | <0.98 | Nb II |
Mo I | 1 | ... | 0.55+-0.27 | -0.10 | -1.98 | 0.55+-0.27 | -0.10 | Mo I |
Tc I | 1 | ... | ... | <0.55 | <0.55 | <3.08 | <0.55 | Tc I |
Sn I | 1 | ... | <1.65 | <1.19 | <-0.88 | <1.65 | <1.19 | Sn I |
Ba II | 2 | ... | -0.40+-0.12 | -0.76 | -2.94 | -0.41+-0.12 | -0.76 | Ba II |
La II | 1 | ... | 0.10+-0.15 | -1.34 | -2.44 | 0.09+-0.15 | -1.34 | La II |
Ce II | 5 | ... | <0.46 | <-0.50 | <-2.08 | <0.45 | <-0.50 | Ce II |
Pr II | 1 | ... | <1.27 | <-0.55 | <-1.27 | <1.26 | <-0.55 | Pr II |
Nd II | 1 | ... | 0.21+-0.20 | -0.91 | -2.33 | 0.20+-0.20 | -0.91 | Nd II |
Sm II | 2 | ... | <0.98 | <-0.60 | <-1.56 | <0.97 | <-0.60 | Sm II |
Eu II | 2 | ... | 0.33+-0.19 | -1.69 | -2.21 | 0.32+-0.19 | -1.69 | Eu II |
Gd II | 2 | ... | <1.12 | <-0.35 | <-1.42 | <1.11 | <-0.35 | Gd II |
Tb II | 3 | ... | <1.29 | <-0.95 | <-1.27 | <1.26 | <-0.95 | Tb II |
Dy II | 1 | ... | 0.62+-0.19 | -0.82 | -1.92 | 0.61+-0.19 | -0.82 | Dy II |
Er II | 3 | ... | <0.88 | <-0.74 | <-1.66 | <0.87 | <-0.74 | Er II |
Tm II | 2 | ... | <1.43 | <-1.01 | <-1.13 | <1.40 | <-1.01 | Tm II |
Yb II | 1 | ... | 0.29+-0.19 | -1.33 | -2.25 | 0.28+-0.19 | -1.33 | Yb II |
Hf II | 2 | ... | <1.84 | <0.15 | <-0.56 | <1.97 | <0.15 | Hf II |
Ir I | 1 | ... | <1.77 | <0.62 | <-0.76 | <1.77 | <0.62 | Ir I |
Pb I | 1 | ... | <1.37 | <0.88 | <-1.16 | <1.37 | <0.88 | Pb I |
Th II | 2 | ... | <1.70 | <-0.78 | <-0.84 | <1.69 | <-0.78 | Th II |
Binarity | Negative |
Vrad | 89.8 |
Right Ascension : 15 09 46.02 | Declination : -04 45 06.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2009-02-21-09:43 | 2454883.906 | MIKELCO | 41000 | 100-315 | 1200 | 90 |
2009-03-16-10:59 | 2454906.961 | HRSHET | 30000 | 100-315 | 1100 | 89.3 |
2009-05-16-05:48 | 2454967.747 | MIKELCO | 41000 | 100-315 | 2100 | 90.1 |