HD51754
HIP33582 in T.Bensby+,AAP, 562, A71, 2014
taken from 6 paper(s):
/J.P.Fulbright(2000)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2009)/
/H.L.Yan et al.(2016)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 5725 | log g : 4.3 | vturb : 1.25 |
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 | ... | 0.06 | ... | -0.59 | 0.13 | 5.65 | Na I |
Mg I | N/A | ... | 0.47 | ... | -0.29 | 0.43 | 7.31 | Mg I |
Si I | N/A | ... | 0.38 | ... | -0.32 | 0.40 | 7.19 | Si I |
Ca I | N/A | ... | 0.24 | ... | -0.48 | 0.24 | 5.86 | Ca I |
Ti | N/A | ... | 0.41 | ... | -0.29 | 0.43 | 4.66 | Ti |
Cr I | N/A | ... | 0.1 | ... | -0.61 | 0.11 | 5.03 | Cr I |
Fe | N/A | -0.74 | ... | ... | -0.72 | ... | 6.78 | Fe |
Ba II | N/A | ... | -0.18 | ... | -0.97 | -0.25 | 1.21 | Ba II |
Position
Right Ascension : 06 58 38.50 | Declination : -00 28 50.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
19990126-31 | N/A | SANDIFORD | 50000 | 65 | 2700 | N/A |
Abundances for metal-poor stars with accurate parallaxes I. Basic data
Stellar Parameters
Teff : 5807 | log g : 4.34 | vturb : 0.74 |
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+-0.054 | ... | -0.62+-0.054 | -0.01+-0.054 | 5.62+-0.054 | Na I |
Mg I | N/A | ... | 0.51+-0.055 | ... | -0.26+-0.055 | 0.35+-0.055 | 7.34+-0.055 | Mg I |
Si I | N/A | ... | 0.23+-0.048 | ... | -0.35+-0.048 | 0.26+-0.048 | 7.16+-0.048 | Si I |
Ca I | N/A | ... | 0.22+-0.033 | ... | -0.45+-0.033 | 0.16+-0.033 | 5.89+-0.033 | Ca I |
Ti II | N/A | ... | 0.29+-0.048 | ... | -0.19+-0.048 | 0.42+-0.048 | 4.76+-0.048 | Ti II |
Fe I | N/A | -0.6+-0.051 | ... | ... | -0.61+-0.051 | ... | 6.89+-0.051 | Fe I |
Fe II | N/A | -0.6+-0.066 | ... | ... | -0.61+-0.066 | ... | 6.89+-0.066 | Fe II |
Position
Right Ascension : 06 58 38.50 | Declination : -00 28 50.0 | 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 | -94.3 |
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 5725 | log g : 4.32 | vturb : 1.25 |
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 | N/A | ... | ... | 1.1 | -2.16 | -1.66 | 1.1 | Li |
Be | N/A | ... | ... | 0.91 | -0.47 | 0.03 | 0.91 | Be |
Fe | N/A | -0.5 | ... | ... | -0.50 | ... | 7.00 | Fe |
Position
Right Ascension : 06 58 38.50 | Declination : -00 28 50.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 5767 | log g : 4.29 | vturb : 1.4 |
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 |
Fe | N/A | -0.58 | ... | ... | -0.58 | ... | 6.92 | Fe |
Cu | N/A | ... | -0.07+-0.03 | ... | -0.63+-0.03 | -0.05+-0.03 | 3.56+-0.03 | Cu |
Position
Right Ascension : 06 58 38.50 | Declination : -00 28 50.0 | 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 | VLT | 55000 | 250-500 | N/A | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5767 | log g : 4.29 | vturb : 1.4 |
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 | ... | 0.11 | ... | -0.38 | 0.20 | 5.86 | Na |
Mg | N/A | ... | 0.33 | ... | -0.27 | 0.31 | 7.33 | Mg |
Si | N/A | ... | 0.25 | ... | -0.29 | 0.29 | 7.22 | Si |
Ca | N/A | ... | 0.24 | ... | -0.32 | 0.26 | 6.02 | Ca |
Ti | N/A | ... | 0.21 | ... | -0.30 | 0.28 | 4.65 | Ti |
Cr | N/A | ... | 0.02 | ... | -0.53 | 0.05 | 5.11 | Cr |
Fe | N/A | -0.58 | ... | ... | -0.58 | ... | 6.92 | Fe |
Ni | N/A | ... | 0.03 | ... | -0.52 | 0.06 | 5.70 | Ni |
Position
Right Ascension : 06 58 38.50 | Declination : -00 28 50.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-11-10-0823 | N/A | VLT | 55000 | 300 | N/A | -94 |
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
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 |
Mn | N/A | ... | -0.17 | ... | -0.79 | -0.21 | 4.64 | Mn |
Fe | N/A | -0.58 | ... | ... | -0.58 | ... | 6.92 | Fe |
Cu | N/A | ... | -0.03 | ... | -0.59 | -0.01 | 3.60 | Cu |
Zn | N/A | ... | 0.14 | ... | -0.40 | 0.18 | 4.16 | Zn |
Y | N/A | ... | -0.15 | ... | -0.70 | -0.12 | 1.51 | Y |
Ba | N/A | ... | -0.23 | ... | -0.86 | -0.28 | 1.32 | Ba |
Position
Right Ascension : 06 58 38.50 | Declination : -00 28 50.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-11-10-0823 | N/A | VLT | 55000 | 300 | N/A | -94 |