G233-26
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 : 5303+-59 | log g : 4.39+-0.26 | vturb : 0.64+-0.18 |
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 | ... | ... | 1.06+-0.05 | -2.20+-0.05 | -0.77+-0.05 | 1.06+-0.05 | Li I |
| Fe | N/A | -1.45+-0.06 | ... | ... | -1.43+-0.06 | ... | 6.07+-0.06 | Fe |
Position
| Right Ascension : 22 39 56.35 | Declination : +61 43 07.6 | 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 | 80 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
| Teff : 5303+-59 | log g : 4.39+-0.26 | vturb : 0.64+-0.18 |
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 | -1.69+-0.18 | -0.23+-0.19 | ... | -1.60+-0.18 | -0.16+-0.19 | 4.64+-0.18 | Na I |
| Mg I | N/A | -1.25+-0.06 | +0.21+-0.09 | ... | -1.27+-0.06 | 0.17+-0.09 | 6.33+-0.06 | Mg I |
| Si | N/A | ... | +0.12+-0.09 | ... | -1.29+-0.09 | 0.15+-0.09 | 6.22+-0.09 | Si |
| Si I | 2 | -1.33+-0.07 | ... | ... | -1.29+-0.07 | 0.15+-0.07 | 6.22+-0.07 | Si I |
| Ca I | N/A | -1.25+-0.09 | +0.20+-0.11 | ... | -1.23+-0.09 | 0.21+-0.11 | 5.11+-0.09 | Ca I |
| Ti | N/A | ... | +0.19+-0.09 | ... | -1.22+-0.09 | 0.22+-0.09 | 3.73+-0.09 | Ti |
| Ti I | 15 | -1.27+-0.09 | ... | ... | -1.23+-0.09 | 0.21+-0.09 | 3.72+-0.09 | Ti I |
| Ti II | 6 | -1.26+-0.08 | ... | ... | -1.22+-0.08 | 0.22+-0.08 | 3.73+-0.08 | Ti II |
| Cr | N/A | ... | -0.02+-0.10 | ... | -1.44+-0.10 | 0.00+-0.10 | 4.20+-0.10 | Cr |
| Cr I | 13 | -1.48+-0.08 | ... | ... | -1.45+-0.08 | -0.01+-0.08 | 4.19+-0.08 | Cr I |
| Cr II | 4 | -1.43+-0.25 | ... | ... | -1.40+-0.25 | 0.04+-0.25 | 4.24+-0.25 | Cr II |
| Fe | N/A | -1.45+-0.06 | ... | ... | -1.44+-0.06 | ... | 6.06+-0.06 | Fe |
| Fe I | 55 | -1.43+-0.07 | ... | ... | -1.42+-0.07 | ... | 6.08+-0.07 | Fe I |
| Fe II | 8 | -1.50+-0.11 | ... | ... | -1.49+-0.11 | ... | 6.01+-0.11 | Fe II |
| Ni I | N/A | -1.62+-0.09 | -0.17+-0.11 | ... | -1.59+-0.09 | -0.15+-0.11 | 4.63+-0.09 | Ni I |
| Y II | N/A | -1.59+-0.24 | -0.13+-0.25 | ... | -1.56+-0.24 | -0.12+-0.25 | 0.65+-0.24 | Y II |
| Ba II | N/A | -1.53+-0.13 | -0.08+-0.14 | ... | -1.58+-0.13 | -0.14+-0.14 | 0.60+-0.13 | Ba II |
Binary Parameters
Position
| Right Ascension : 22 39 56.35 | Declination : +61 43 07.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2450987.604 | KECKHIRES | 48000 | 80 | 1200 | -313.6+-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 | ... | -0.23 | ... | -1.59 | -0.14 | 4.65 | Na |
| Mg | N/A | ... | 0.21 | ... | -1.26 | 0.19 | 6.34 | Mg |
| Ca | N/A | ... | 0.2 | ... | -1.23 | 0.22 | 5.11 | Ca |
| Ti | N/A | ... | 0.19 | ... | -1.19 | 0.26 | 3.76 | Ti |
| Fe | N/A | -1.45 | ... | ... | -1.45 | ... | 6.05 | Fe |
| Ni | N/A | ... | -0.17 | ... | -1.59 | -0.14 | 4.63 | Ni |
| Y | N/A | ... | -0.21 | ... | -1.63 | -0.18 | 0.58 | Y |
| Ba | N/A | ... | -0.08 | ... | -1.58 | -0.13 | 0.60 | Ba |
Position
| Right Ascension : 22 39 56.35 | Declination : +61 43 07.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log