G5-19
taken from 8 paper(s):
/R.Smiljanic et al.(2009)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/H.L.Yan et al.(2016)/
/A.M.Boesgaard et al.(2011)/
/K.A.Venn et al.(2004)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 5942 | log g : 4.24 | vturb : 0.89 |
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 | ... | ... | 2.26 | -1.00 | 0.10 | 2.26 | Li |
Be | N/A | ... | ... | -0.01 | -1.39 | -0.29 | -0.01 | Be |
Fe | N/A | -1.1 | ... | ... | -1.10 | ... | 6.40 | Fe |
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 5942+-56 | log g : 4.24+-0.24 | vturb : 0.89+-0.11 |
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 | N/A | ... | ... | 2.26+-0.05 | -1.00+-0.05 | 0.08+-0.05 | 2.26+-0.05 | Li I |
Fe | N/A | -1.10+-0.08 | ... | ... | -1.08+-0.08 | ... | 6.42+-0.08 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 110 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 5942+-56 | log g : 4.24+-0.24 | vturb : 0.89+-0.11 |
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 | -1.37+-0.20 | -0.21+-0.20 | ... | -1.28+-0.20 | -0.13+-0.20 | 4.96+-0.20 | Na I |
Mg I | N/A | -0.96+-0.09 | +0.20+-0.10 | ... | -0.98+-0.09 | 0.17+-0.10 | 6.62+-0.09 | Mg I |
Si | N/A | ... | +0.12+-0.10 | ... | -1.00+-0.10 | 0.15+-0.10 | 6.51+-0.10 | Si |
Si I | 3 | -0.97+-0.12 | ... | ... | -0.93+-0.12 | 0.22+-0.12 | 6.58+-0.12 | Si I |
Si II | 1 | -1.17+-0.16 | ... | ... | -1.13+-0.16 | 0.02+-0.16 | 6.38+-0.16 | Si II |
Ca I | N/A | -0.97+-0.08 | +0.19+-0.09 | ... | -0.95+-0.08 | 0.20+-0.09 | 5.39+-0.08 | Ca I |
Ti | N/A | ... | +0.22+-0.09 | ... | -0.90+-0.09 | 0.25+-0.09 | 4.05+-0.09 | Ti |
Ti I | 16 | -1.00+-0.12 | ... | ... | -0.96+-0.12 | 0.19+-0.12 | 3.99+-0.12 | Ti I |
Ti II | 8 | -0.90+-0.10 | ... | ... | -0.86+-0.10 | 0.29+-0.10 | 4.09+-0.10 | Ti II |
Cr | N/A | ... | +0.00+-0.08 | ... | -1.13+-0.08 | 0.02+-0.08 | 4.51+-0.08 | Cr |
Cr I | 14 | -1.18+-0.08 | ... | ... | -1.15+-0.08 | 0.00+-0.08 | 4.49+-0.08 | Cr I |
Cr II | 5 | -1.06+-0.17 | ... | ... | -1.03+-0.17 | 0.12+-0.17 | 4.61+-0.17 | Cr II |
Fe | N/A | -1.16+-0.04 | ... | ... | -1.15+-0.04 | ... | 6.35+-0.04 | Fe |
Fe I | 71 | -1.09+-0.08 | ... | ... | -1.08+-0.08 | ... | 6.42+-0.08 | Fe I |
Fe II | 10 | -1.18+-0.05 | ... | ... | -1.17+-0.05 | ... | 6.33+-0.05 | Fe II |
Ni I | N/A | -1.26+-0.13 | -0.10+-0.13 | ... | -1.23+-0.13 | -0.08+-0.13 | 4.99+-0.13 | Ni I |
Y II | N/A | -1.21+-0.05 | -0.05+-0.07 | ... | -1.18+-0.05 | -0.03+-0.07 | 1.03+-0.05 | Y II |
Ba II | N/A | -1.01+-0.13 | +0.15+-0.14 | ... | -1.06+-0.13 | 0.09+-0.14 | 1.12+-0.13 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2451067.648 | KECKHIRES | 48000 | 110 | 200 | -215.6+-0.6 |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 5854 | log g : 4.26 | vturb : 1.3 |
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 | -1.18 | ... | ... | -1.18 | ... | 6.32 | Fe |
Cu | N/A | ... | -0.70+-0.00 | ... | -1.86+-0.00 | -0.68+-0.00 | 2.33+-0.00 | Cu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 55000 | 250-500 | N/A | N/A |
Beryllium and Alpha-element Abundances in a Large Sample of Metal-poor Stars
Stellar Parameters
Teff : 5975+-100 | log g : 3.93+-0.2 | vturb : 1.34+-0.2 |
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 |
Be | N/A | ... | -0.37+-0.15 | -0.08+-0.12 | -1.46+-0.12 | -0.33+-0.15 | -0.08+-0.12 | Be |
O | N/A | -0.62+-0.22 | +0.51+-0.24 | ... | -0.68+-0.22 | 0.45+-0.24 | 8.01+-0.22 | O |
Mg | N/A | -0.88+-0.07 | ... | ... | -0.90+-0.07 | 0.23+-0.07 | 6.70+-0.07 | Mg |
Ti | N/A | -1.02+-0.09 | ... | ... | -0.95+-0.09 | 0.18+-0.09 | 4.00+-0.09 | Ti |
Fe | N/A | -1.13+-0.09 | ... | ... | -1.13+-0.09 | ... | 6.37+-0.09 | Fe |
Position
Right Ascension : | Declination : | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-09-27 | N/A | KECKHIRES | 42000 | 90 | 3600 | N/A |
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 | ... | -0.21 | ... | -1.28 | -0.12 | 4.96 | Na |
Mg | N/A | ... | 0.2 | ... | -0.98 | 0.18 | 6.62 | Mg |
Ca | N/A | ... | 0.19 | ... | -0.95 | 0.21 | 5.39 | Ca |
Ti | N/A | ... | 0.22 | ... | -0.87 | 0.29 | 4.08 | Ti |
Fe | N/A | -1.16 | ... | ... | -1.16 | ... | 6.34 | Fe |
Ni | N/A | ... | -0.1 | ... | -1.23 | -0.07 | 4.99 | Ni |
Y | N/A | ... | -0.14 | ... | -1.27 | -0.11 | 0.94 | Y |
Ba | N/A | ... | 0.15 | ... | -1.06 | 0.10 | 1.12 | Ba |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5854 | log g : 4.26 | vturb : 1.3 |
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 | ... | -0.25 | ... | -1.34 | -0.16 | 4.90 | Na |
Mg | N/A | ... | 0.18 | ... | -1.02 | 0.16 | 6.58 | Mg |
Si | N/A | ... | 0.17 | ... | -0.97 | 0.21 | 6.54 | Si |
Ca | N/A | ... | 0.26 | ... | -0.90 | 0.28 | 5.44 | Ca |
Ti | N/A | ... | 0.14 | ... | -0.97 | 0.21 | 3.98 | Ti |
Cr | N/A | ... | -0.05 | ... | -1.20 | -0.02 | 4.44 | Cr |
Fe | N/A | -1.18 | ... | ... | -1.18 | ... | 6.32 | Fe |
Ni | N/A | ... | -0.13 | ... | -1.28 | -0.10 | 4.94 | Ni |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-10-15-0521 | N/A | VLT | 55000 | 300 | N/A | -216.2 |
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 | ... | -0.35 | ... | -1.57 | -0.39 | 3.86 | Mn |
Fe | N/A | -1.18 | ... | ... | -1.18 | ... | 6.32 | Fe |
Cu | N/A | ... | -0.62 | ... | -1.78 | -0.60 | 2.41 | Cu |
Zn | N/A | ... | 0.01 | ... | -1.13 | 0.05 | 3.43 | Zn |
Y | N/A | ... | -0.12 | ... | -1.27 | -0.09 | 0.94 | Y |
Ba | N/A | ... | -0.17 | ... | -1.40 | -0.22 | 0.78 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-10-15-0521 | N/A | VLT | 55000 | 300 | N/A | -216.2 |