G84-29
taken from 4 paper(s):
/J.R.Shi et al.(2007)/
/I.I.Ivans et al.(2003)/
/T.Gehren et al.(2006)/
/D.Fabbian et al.(2009)/
Lithium abundances in metal-poor stars (Research Note)
Stellar Parameters
Teff : 6240 | log g : 4.14 | vturb : 1.60 |
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 | ... | ... | 2.19 | -1.07 | 1.37 | 2.19 | Li I |
Fe | N/A | -2.45 | ... | ... | -2.44 | ... | 5.06 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 100-400 | N/A | N/A |
Chemical Substructure in the Milky Way Halo: A New Population of Old Stars
Stellar Parameters
Teff : 6330 | log g : 3.55 | vturb : 1.40 |
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 | ... | ... | <2.58 | <-0.68 | <2.06 | <2.58 | Li I |
O I | N/A | ... | <+0.66 | ... | <-1.86 | <0.88 | <6.83 | O I |
Na I | 2 | ... | -0.26+-0.00 | ... | -2.93+-0.00 | -0.19+-0.00 | 3.31+-0.00 | Na I |
Mg I | 2 | ... | +0.40+-0.20 | ... | -2.38+-0.20 | 0.36+-0.20 | 5.22+-0.20 | Mg I |
Ca I | 6 | ... | +0.37+-0.09 | ... | -2.37+-0.09 | 0.37+-0.09 | 3.97+-0.09 | Ca I |
Sc II | 1 | ... | +0.31 | ... | -2.51 | 0.23 | 0.64 | Sc II |
Ti I | 4 | ... | +0.76+-0.15 | ... | -1.96+-0.15 | 0.78+-0.15 | 2.99+-0.15 | Ti I |
Ti II | 3 | ... | +0.55+-0.09 | ... | -2.17+-0.09 | 0.57+-0.09 | 2.78+-0.09 | Ti II |
V I | N/A | ... | <+2.60 | ... | <-0.09 | <2.65 | <3.84 | V I |
Cr I | 3 | ... | +0.08+-0.20 | ... | -2.65+-0.20 | 0.09+-0.20 | 2.99+-0.20 | Cr I |
Mn I | 1 | ... | +0.38 | ... | -2.42 | 0.32 | 3.01 | Mn I |
Fe I | 38 | -2.76+-0.12 | ... | ... | -2.74+-0.12 | ... | 4.76+-0.12 | Fe I |
Fe II | 5 | -2.74+-0.07 | ... | ... | -2.72+-0.07 | ... | 4.78+-0.07 | Fe II |
Ni I | 4 | ... | +0.42+-0.35 | ... | -2.31+-0.35 | 0.43+-0.35 | 3.91+-0.35 | Ni I |
Cu I | N/A | ... | <+1.40 | ... | <-1.34 | <1.40 | <2.85 | Cu I |
Y II | N/A | ... | <+0.83 | ... | <-1.90 | <0.84 | <0.31 | Y II |
Ba II | N/A | ... | <+0.16 | ... | <-2.65 | <0.09 | <-0.47 | Ba II |
Eu II | N/A | ... | <+2.63 | ... | <-0.14 | <2.60 | <0.38 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-11-09 | N/A | MAYALLKPNO | 28000 | 100-150 | 1200 | N/A |
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 6240 | log g : 4.14+-0.28 | vturb : 1.6 |
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 | 2 | ... | -0.50 | ... | -2.86 | -0.42 | 3.38 | Na I |
Mg I | 4 | ... | -0.07 | ... | -2.54 | -0.10 | 5.06 | Mg I |
Fe | N/A | -2.45 | ... | ... | -2.44 | ... | 5.06 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 200 | 3600 | N/A |
The C/O ratio at low metallicity:constraints on early chemical evolution from observations of Galactic halo stars
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 |
C | N/A | -2.33 | ... | 6.06 | -2.37 | 0.30 | 6.06 | C |
O | N/A | -1.79 | ... | 6.87 | -1.82 | 0.85 | 6.87 | O |
Fe | N/A | -2.62 | ... | ... | -2.67 | ... | 4.83 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-12 | N/A | MIKELCO | 60000 | 40-500 | N/A | N/A |