HD118659
HIP66509 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 3 paper(s):
/J.P.Fulbright(2000)/
/R.G.Gratton et al.(2003)/
/T.Gehren et al.(2006)/
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 5350 | log g : 4.2 | vturb : 0.6 |
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 |
Na I | N/A | ... | 0.01 | ... | -0.58 | 0.08 | 5.66 | Na I |
Mg I | N/A | ... | 0.36 | ... | -0.34 | 0.32 | 7.26 | Mg I |
Al I | N/A | ... | 0.28 | ... | -0.38 | 0.28 | 6.07 | Al I |
Si I | N/A | ... | 0.27 | ... | -0.37 | 0.29 | 7.14 | Si I |
Ca I | N/A | ... | 0.2 | ... | -0.46 | 0.20 | 5.88 | Ca I |
Ti | N/A | ... | 0.19 | ... | -0.45 | 0.21 | 4.50 | Ti |
V I | N/A | ... | 0.11 | ... | -0.50 | 0.16 | 3.43 | V I |
Cr I | N/A | ... | 0.03 | ... | -0.62 | 0.04 | 5.02 | Cr I |
Fe | N/A | -0.68 | ... | ... | -0.66 | ... | 6.84 | Fe |
Ni I | N/A | ... | 0.06 | ... | -0.59 | 0.07 | 5.63 | Ni I |
Y II | N/A | ... | -0.16 | ... | -0.81 | -0.15 | 1.40 | Y II |
Zr II | N/A | ... | 0.02 | ... | -0.64 | 0.02 | 1.94 | Zr II |
Ba II | N/A | ... | -0.07 | ... | -0.80 | -0.14 | 1.38 | Ba II |
Eu II | N/A | ... | 0.25 | ... | -0.44 | 0.22 | 0.08 | Eu II |
Position
Right Ascension : 13 38 00.47 | Declination : +19 08 53.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1995-06-10 | N/A | LICKHAMILTON | 50000 | 125 | 1000 | N/A |
Abundances for metal-poor stars with accurate parallaxes I. Basic data
Stellar Parameters
Teff : 5446 | log g : 4.35 | vturb : 0.6 |
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 |
Na I | N/A | ... | 0.05+-0.054 | ... | -0.63+-0.054 | 0.03+-0.054 | 5.61+-0.054 | Na I |
Mg I | N/A | ... | 0.33+-0.055 | ... | -0.49+-0.055 | 0.17+-0.055 | 7.11+-0.055 | Mg I |
Si I | N/A | ... | 0.19+-0.048 | ... | -0.44+-0.048 | 0.22+-0.048 | 7.07+-0.048 | Si I |
Ca I | N/A | ... | 0.21+-0.033 | ... | -0.51+-0.033 | 0.15+-0.033 | 5.83+-0.033 | Ca I |
Ti I | N/A | ... | 0.19+-0.03 | ... | -0.34+-0.03 | 0.32+-0.03 | 4.61+-0.03 | Ti I |
Ti II | N/A | ... | 0.12+-0.048 | ... | -0.41+-0.048 | 0.25+-0.048 | 4.54+-0.048 | Ti II |
Fe I | N/A | -0.65+-0.051 | ... | ... | -0.66+-0.051 | ... | 6.84+-0.051 | Fe I |
Fe II | N/A | -0.68+-0.066 | ... | ... | -0.69+-0.066 | ... | 6.81+-0.066 | Fe II |
Position
Right Ascension : 13 38 00.47 | Declination : +19 08 53.1 | 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 | N/A | 50000 | >100 | N/A | -45.3 |
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 5510 | log g : 4.36+-0.10 | vturb : 1.0 |
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 I | 6 | ... | 0.20 | ... | -0.31 | 0.28 | 5.93 | Na I |
Mg I | 7 | ... | 0.33 | ... | -0.29 | 0.30 | 7.31 | Mg I |
Al I | 7 | ... | 0.24 | ... | -0.34 | 0.25 | 6.11 | Al I |
Fe | N/A | -0.60 | ... | ... | -0.59 | ... | 6.91 | Fe |
Position
Right Ascension : 13 38 00.47 | Declination : +19 08 53.1 | 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 | FOCES | 40000 | 200 | 5800 | N/A |