G121-12
taken from 5 paper(s):
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/H.L.Yan et al.(2016)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 6163+-67 | log g : 4.37+-0.30 | vturb : 1.06+-0.07 |
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 | ... | ... | 2.59+-0.05 | -0.67+-0.05 | 0.10+-0.05 | 2.59+-0.05 | Li I |
Fe | N/A | -0.79+-0.06 | ... | ... | -0.77+-0.06 | ... | 6.73+-0.06 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 185 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 6163+-67 | log g : 4.37+-0.30 | vturb : 1.06+-0.07 |
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 | -1.09+-0.12 | -0.29+-0.13 | ... | -1.00+-0.12 | -0.21+-0.13 | 5.24+-0.12 | Na I |
Mg I | N/A | -0.74+-0.05 | +0.06+-0.08 | ... | -0.76+-0.05 | 0.03+-0.08 | 6.84+-0.05 | Mg I |
Si | N/A | ... | -0.02+-0.08 | ... | -0.78+-0.08 | 0.01+-0.08 | 6.73+-0.08 | Si |
Si I | 3 | -0.80+-0.07 | ... | ... | -0.76+-0.07 | 0.03+-0.07 | 6.75+-0.07 | Si I |
Si II | 1 | -0.93+-0.16 | ... | ... | -0.89+-0.16 | -0.10+-0.16 | 6.62+-0.16 | Si II |
Ca I | N/A | -0.70+-0.09 | +0.10+-0.11 | ... | -0.68+-0.09 | 0.11+-0.11 | 5.66+-0.09 | Ca I |
Ti | N/A | ... | +0.13+-0.09 | ... | -0.63+-0.09 | 0.16+-0.09 | 4.32+-0.09 | Ti |
Ti I | 23 | -0.72+-0.11 | ... | ... | -0.68+-0.11 | 0.11+-0.11 | 4.27+-0.11 | Ti I |
Ti II | 8 | -0.61+-0.11 | ... | ... | -0.57+-0.11 | 0.22+-0.11 | 4.38+-0.11 | Ti II |
Cr | N/A | ... | -0.05+-0.07 | ... | -0.82+-0.07 | -0.03+-0.07 | 4.82+-0.07 | Cr |
Cr I | 13 | -0.86+-0.04 | ... | ... | -0.83+-0.04 | -0.04+-0.04 | 4.81+-0.04 | Cr I |
Cr II | 5 | -0.78+-0.13 | ... | ... | -0.75+-0.13 | 0.04+-0.13 | 4.89+-0.13 | Cr II |
Fe | N/A | -0.80+-0.06 | ... | ... | -0.79+-0.06 | ... | 6.71+-0.06 | Fe |
Fe I | 69 | -0.77+-0.07 | ... | ... | -0.76+-0.07 | ... | 6.74+-0.07 | Fe I |
Fe II | 10 | -0.85+-0.10 | ... | ... | -0.84+-0.10 | ... | 6.66+-0.10 | Fe II |
Ni I | N/A | -1.01+-0.10 | -0.22+-0.12 | ... | -0.98+-0.10 | -0.19+-0.12 | 5.24+-0.10 | Ni I |
Y II | N/A | -0.90+-0.05 | -0.10+-0.07 | ... | -0.87+-0.05 | -0.08+-0.07 | 1.34+-0.05 | Y II |
Ba II | N/A | -0.65+-0.09 | +0.15+-0.10 | ... | -0.70+-0.09 | 0.09+-0.10 | 1.48+-0.09 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2450595.26 | KECKHIRES | 48000 | 185 | 300 | 198.3+-0.5 |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 5928 | log g : 4.23 | 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 | -0.93 | ... | ... | -0.93 | ... | 6.57 | Fe |
Cu | N/A | ... | -0.73+-0.00 | ... | -1.64+-0.00 | -0.71+-0.00 | 2.55+-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 |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5928 | log g : 4.23 | 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 | ... | -0.3 | ... | -1.14 | -0.21 | 5.10 | Na |
Mg | N/A | ... | 0.03 | ... | -0.92 | 0.01 | 6.68 | Mg |
Si | N/A | ... | 0.1 | ... | -0.79 | 0.14 | 6.72 | Si |
Ca | N/A | ... | 0.19 | ... | -0.72 | 0.21 | 5.62 | Ca |
Ti | N/A | ... | 0.08 | ... | -0.78 | 0.15 | 4.17 | Ti |
Cr | N/A | ... | -0.04 | ... | -0.94 | -0.01 | 4.70 | Cr |
Fe | N/A | -0.93 | ... | ... | -0.93 | ... | 6.57 | Fe |
Ni | N/A | ... | -0.19 | ... | -1.09 | -0.16 | 5.13 | Ni |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-01-14-0714 | N/A | VLT | 55000 | 300 | N/A | 197.4 |
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 | ... | -0.33 | ... | -1.30 | -0.37 | 4.13 | Mn |
Fe | N/A | -0.93 | ... | ... | -0.93 | ... | 6.57 | Fe |
Cu | N/A | ... | -0.75 | ... | -1.66 | -0.73 | 2.53 | Cu |
Zn | N/A | ... | -0.12 | ... | -1.01 | -0.08 | 3.55 | Zn |
Y | N/A | ... | -0.17 | ... | -1.07 | -0.14 | 1.14 | Y |
Ba | N/A | ... | -0.14 | ... | -1.12 | -0.19 | 1.06 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-01-14-0714 | N/A | VLT | 55000 | 300 | N/A | 197.4 |