HD149996
HIP81461 in T.Bensby+,AAP, 562, A71, 2014
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 : 5600 | log g : 4.1 | vturb : 1.2 |
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 |
Na I | N/A | ... | 0.18 | ... | -0.38 | 0.25 | 5.86 | Na I |
Mg I | N/A | ... | 0.47 | ... | -0.20 | 0.43 | 7.40 | Mg I |
Al I | N/A | ... | 0.39 | ... | -0.24 | 0.39 | 6.21 | Al I |
Si I | N/A | ... | 0.41 | ... | -0.20 | 0.43 | 7.31 | Si I |
Ca I | N/A | ... | 0.25 | ... | -0.38 | 0.25 | 5.96 | Ca I |
Ti | N/A | ... | 0.3 | ... | -0.31 | 0.32 | 4.64 | Ti |
V I | N/A | ... | 0.08 | ... | -0.50 | 0.13 | 3.43 | V I |
Cr I | N/A | ... | 0.07 | ... | -0.55 | 0.08 | 5.09 | Cr I |
Fe | N/A | -0.65 | ... | ... | -0.63 | ... | 6.87 | Fe |
Ni I | N/A | ... | 0.1 | ... | -0.52 | 0.11 | 5.70 | Ni I |
Y II | N/A | ... | -0.01 | ... | -0.63 | 0.00 | 1.58 | Y II |
Zr II | N/A | ... | 0.1 | ... | -0.53 | 0.10 | 2.05 | Zr II |
Ba II | N/A | ... | 0.01 | ... | -0.69 | -0.06 | 1.49 | Ba II |
Eu II | N/A | ... | 0.55 | ... | -0.11 | 0.52 | 0.41 | Eu II |
Position
Right Ascension : 16 38 17.39 | Declination : -02 26 31.8 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-08-08 | N/A | LICKHAMILTON | 50000 | 100 | 900 | N/A |
Abundances for metal-poor stars with accurate parallaxes I. Basic data
Stellar Parameters
Teff : 5660 | log g : 4.08 | vturb : 0.95 |
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 | ... | 0.16+-0.054 | ... | -0.44+-0.054 | 0.14+-0.054 | 5.80+-0.054 | Na I |
Mg I | N/A | ... | 0.49+-0.055 | ... | -0.25+-0.055 | 0.33+-0.055 | 7.35+-0.055 | Mg I |
Si I | N/A | ... | 0.29+-0.048 | ... | -0.26+-0.048 | 0.32+-0.048 | 7.25+-0.048 | Si I |
Ca I | N/A | ... | 0.26+-0.033 | ... | -0.38+-0.033 | 0.20+-0.033 | 5.96+-0.033 | Ca I |
Ti I | N/A | ... | 0.25+-0.03 | ... | -0.20+-0.03 | 0.38+-0.03 | 4.75+-0.03 | Ti I |
Ti II | N/A | ... | 0.18+-0.048 | ... | -0.27+-0.048 | 0.31+-0.048 | 4.68+-0.048 | Ti II |
Fe I | N/A | -0.57+-0.051 | ... | ... | -0.58+-0.051 | ... | 6.92+-0.051 | Fe I |
Fe II | N/A | -0.66+-0.066 | ... | ... | -0.67+-0.066 | ... | 6.83+-0.066 | Fe II |
Position
Right Ascension : 16 38 17.39 | Declination : -02 26 31.8 | 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 | -35.9 |
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 5665 | log g : 4.09+-0.12 | vturb : 1.2 |
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 |
Na I | 6 | ... | 0.20 | ... | -0.23 | 0.28 | 6.01 | Na I |
Mg I | 7 | ... | 0.30 | ... | -0.24 | 0.27 | 7.36 | Mg I |
Al I | 7 | ... | 0.19 | ... | -0.31 | 0.20 | 6.14 | Al I |
Fe | N/A | -0.52 | ... | ... | -0.51 | ... | 6.99 | Fe |
Position
Right Ascension : 16 38 17.39 | Declination : -02 26 31.8 | 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 | 3600 | N/A |