G189-50
taken from 3 paper(s):
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/K.A.Venn et al.(2004)/
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 5254+-82 | log g : 4.32+-0.28 | vturb : 0.26+-0.34 |
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 | ... | ... | 1.46+-0.06 | -1.80+-0.06 | -0.36+-0.06 | 1.46+-0.06 | Li I |
Fe | N/A | -1.46+-0.06 | ... | ... | -1.44+-0.06 | ... | 6.06+-0.06 | Fe |
Position
Right Ascension : 22 56 27.49 | Declination : +33 53 04.2 | 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 | KECKHIRES | 48000 | 180 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 5254+-82 | log g : 4.32+-0.28 | vturb : 0.26+-0.34 |
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 | -1.84+-0.18 | -0.37+-0.19 | ... | -1.75+-0.18 | -0.29+-0.19 | 4.49+-0.18 | Na I |
Mg I | N/A | -1.32+-0.13 | +0.15+-0.14 | ... | -1.34+-0.13 | 0.12+-0.14 | 6.26+-0.13 | Mg I |
Si | N/A | ... | +0.14+-0.12 | ... | -1.29+-0.12 | 0.17+-0.12 | 6.22+-0.12 | Si |
Si I | 1 | -1.47+-0.16 | ... | ... | -1.43+-0.16 | 0.03+-0.16 | 6.08+-0.16 | Si I |
Si II | 1 | -1.20+-0.16 | ... | ... | -1.16+-0.16 | 0.30+-0.16 | 6.35+-0.16 | Si II |
Ca I | N/A | -1.36+-0.10 | +0.11+-0.11 | ... | -1.34+-0.10 | 0.12+-0.11 | 5.00+-0.10 | Ca I |
Ti | N/A | ... | +0.09+-0.08 | ... | -1.34+-0.08 | 0.12+-0.08 | 3.61+-0.08 | Ti |
Ti I | 22 | -1.43+-0.08 | ... | ... | -1.39+-0.08 | 0.07+-0.08 | 3.56+-0.08 | Ti I |
Ti II | 6 | -1.32+-0.10 | ... | ... | -1.28+-0.10 | 0.18+-0.10 | 3.67+-0.10 | Ti II |
Cr | N/A | ... | +0.00+-0.08 | ... | -1.44+-0.08 | 0.02+-0.08 | 4.20+-0.08 | Cr |
Cr I | 14 | -1.50+-0.07 | ... | ... | -1.47+-0.07 | -0.01+-0.07 | 4.17+-0.07 | Cr I |
Cr II | 5 | -1.36+-0.15 | ... | ... | -1.33+-0.15 | 0.13+-0.15 | 4.31+-0.15 | Cr II |
Fe | N/A | -1.47+-0.05 | ... | ... | -1.46+-0.05 | ... | 6.04+-0.05 | Fe |
Fe I | 60 | -1.45+-0.06 | ... | ... | -1.44+-0.06 | ... | 6.06+-0.06 | Fe I |
Fe II | 12 | -1.52+-0.09 | ... | ... | -1.51+-0.09 | ... | 5.99+-0.09 | Fe II |
Ni I | N/A | -1.66+-0.15 | -0.19+-0.16 | ... | -1.63+-0.15 | -0.17+-0.16 | 4.59+-0.15 | Ni I |
Y II | N/A | -1.75+-0.05 | -0.28+-0.07 | ... | -1.72+-0.05 | -0.26+-0.07 | 0.49+-0.05 | Y II |
Ba II | N/A | -1.54+-0.10 | -0.07+-0.12 | ... | -1.59+-0.10 | -0.13+-0.12 | 0.59+-0.10 | Ba II |
Binary Parameters
Position
Right Ascension : 22 56 27.49 | Declination : +33 53 04.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2451067.459 | KECKHIRES | 48000 | 180 | 1800 | -320.7+-0.6 |
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 | ... | -0.37 | ... | -1.75 | -0.28 | 4.49 | Na |
Mg | N/A | ... | 0.15 | ... | -1.34 | 0.13 | 6.26 | Mg |
Ca | N/A | ... | 0.11 | ... | -1.34 | 0.13 | 5.00 | Ca |
Ti | N/A | ... | 0.09 | ... | -1.31 | 0.16 | 3.64 | Ti |
Fe | N/A | -1.47 | ... | ... | -1.47 | ... | 6.03 | Fe |
Ni | N/A | ... | -0.19 | ... | -1.63 | -0.16 | 4.59 | Ni |
Y | N/A | ... | -0.37 | ... | -1.81 | -0.34 | 0.40 | Y |
Ba | N/A | ... | -0.07 | ... | -1.59 | -0.12 | 0.59 | Ba |
Position
Right Ascension : 22 56 27.49 | Declination : +33 53 04.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log