G18-40
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 : 5681+-67 | log g : 4.18+-0.34 | vturb : 1.27+-0.09 |
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 | ... | ... | 2.09+-0.05 | -1.17+-0.05 | 0.72+-0.05 | 2.09+-0.05 | Li I |
| Fe | N/A | -1.91+-0.05 | ... | ... | -1.89+-0.05 | ... | 5.61+-0.05 | Fe |
Position
| Right Ascension : 22 19 53.62 | Declination : +05 25 47.3 | 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 | 140 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
| Teff : 5681+-67 | log g : 4.18+-0.34 | vturb : 1.27+-0.09 |
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 | -2.23+-0.15 | -0.30+-0.16 | ... | -2.14+-0.15 | -0.22+-0.16 | 4.10+-0.15 | Na I |
| Mg I | N/A | -1.63+-0.05 | +0.30+-0.08 | ... | -1.65+-0.05 | 0.27+-0.08 | 5.95+-0.05 | Mg I |
| Si | N/A | ... | +0.22+-0.12 | ... | -1.67+-0.12 | 0.25+-0.12 | 5.84+-0.12 | Si |
| Si I | 3 | -1.71+-0.11 | ... | ... | -1.67+-0.11 | 0.25+-0.11 | 5.84+-0.11 | Si I |
| Ca I | N/A | -1.66+-0.10 | +0.27+-0.11 | ... | -1.64+-0.10 | 0.28+-0.11 | 4.70+-0.10 | Ca I |
| Ti | N/A | ... | +0.24+-0.07 | ... | -1.65+-0.07 | 0.27+-0.07 | 3.30+-0.07 | Ti |
| Ti I | 7 | -1.77+-0.07 | ... | ... | -1.73+-0.07 | 0.19+-0.07 | 3.22+-0.07 | Ti I |
| Ti II | 7 | -1.65+-0.05 | ... | ... | -1.61+-0.05 | 0.31+-0.05 | 3.34+-0.05 | Ti II |
| Cr | N/A | ... | -0.04+-0.10 | ... | -1.94+-0.10 | -0.02+-0.10 | 3.70+-0.10 | Cr |
| Cr I | 13 | -2.00+-0.09 | ... | ... | -1.97+-0.09 | -0.05+-0.09 | 3.67+-0.09 | Cr I |
| Cr II | 5 | -1.87+-0.17 | ... | ... | -1.84+-0.17 | 0.08+-0.17 | 3.80+-0.17 | Cr II |
| Fe | N/A | -1.93+-0.06 | ... | ... | -1.92+-0.06 | ... | 5.58+-0.06 | Fe |
| Fe I | 56 | -1.90+-0.07 | ... | ... | -1.89+-0.07 | ... | 5.61+-0.07 | Fe I |
| Fe II | 9 | -2.00+-0.10 | ... | ... | -1.99+-0.10 | ... | 5.51+-0.10 | Fe II |
| Ni I | N/A | -2.03+-0.11 | -0.10+-0.13 | ... | -2.00+-0.11 | -0.08+-0.13 | 4.22+-0.11 | Ni I |
| Y II | N/A | -2.20+-0.15 | -0.27+-0.16 | ... | -2.17+-0.15 | -0.25+-0.16 | 0.04+-0.15 | Y II |
| Ba II | N/A | -1.97+-0.12 | -0.04+-0.13 | ... | -2.02+-0.12 | -0.10+-0.13 | 0.16+-0.12 | Ba II |
Binary Parameters
Position
| Right Ascension : 22 19 53.62 | Declination : +05 25 47.3 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2450987.553 | KECKHIRES | 48000 | 140 | 2700 | -191.5+-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 | ... | -0.3 | ... | -2.14 | -0.21 | 4.10 | Na |
| Mg | N/A | ... | 0.3 | ... | -1.65 | 0.28 | 5.95 | Mg |
| Ca | N/A | ... | 0.27 | ... | -1.64 | 0.29 | 4.70 | Ca |
| Ti | N/A | ... | 0.24 | ... | -1.62 | 0.31 | 3.33 | Ti |
| Fe | N/A | -1.93 | ... | ... | -1.93 | ... | 5.57 | Fe |
| Ni | N/A | ... | -0.1 | ... | -2.00 | -0.07 | 4.22 | Ni |
| Y | N/A | ... | -0.36 | ... | -2.26 | -0.33 | -0.05 | Y |
| Ba | N/A | ... | -0.04 | ... | -2.02 | -0.09 | 0.16 | Ba |
Position
| Right Ascension : 22 19 53.62 | Declination : +05 25 47.3 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log