BD-4_3208
taken from 3 paper(s):
/M.Bergemann et al.(2010)/
/M.Bergemann and G. Cescutti(2010)/
/C.Sneden et al.(2023)/
NLTE analysis of Co i /Co ii lines in spectra of cool stars with new laboratory hyperfine splitting constants
Stellar Parameters
| Teff : 6310+-60 | log g : 3.98+-0.21 | vturb : 1.5 |
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 | -2.23 | ... | ... | -2.23 | ... | 5.27 | Fe |
| Co | 2 | ... | 0.13+-0.01 | ... | -2.10+-0.01 | 0.13+-0.01 | 2.89+-0.01 | Co |
Position
| Right Ascension : 12 07 15.07 | Declination : -05 44 01.6 | 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 | VLT | N/A | N/A | N/A | N/A |
Chromium: NLTE abundances in metal-poor stars and nucleosynthesis in the Galaxy
Stellar Parameters
| Teff : 6310+-100 | log g : 3.98+-0.05 | vturb : 1.5+-0.2 |
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 |
|---|
| Cr I | 6 | ... | -0.24+-0.03 | ... | -2.45+-0.03 | -0.22+-0.03 | 3.19+-0.03 | Cr I |
| Fe | N/A | -2.23 | ... | ... | -2.23 | ... | 5.27 | Fe |
Position
| Right Ascension : 12 07 15.07 | Declination : -05 44 01.6 | 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 | FOCES | 40000 | N/A | N/A | N/A |
| 2001 | N/A | VLT | 40000 | N/A | N/A | N/A |
Iron-peak Element Abundances in Warm Very Metal-poor Stars
Stellar Parameters
| Teff : 6200 | log g : 3.65 | vturb : 1.45 |
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 |
|---|
| Mg I | 5 | ... | 0.53+-0.09 | ... | -2.02+-0.09 | 0.53+-0.09 | 5.58+-0.09 | Mg I |
| Ca I | 22 | ... | 0.55+-0.05 | ... | -2.00+-0.05 | 0.55+-0.05 | 4.34+-0.05 | Ca I |
| Sc II | 13 | ... | 0.16+-0.06 | ... | -2.39+-0.06 | 0.16+-0.06 | 0.76+-0.06 | Sc II |
| Ti I | 13 | ... | 0.55+-0.07 | ... | -2.00+-0.07 | 0.55+-0.07 | 2.95+-0.07 | Ti I |
| Ti II | 66 | ... | 0.4+-0.14 | ... | -2.15+-0.14 | 0.40+-0.14 | 2.80+-0.14 | Ti II |
| V II | 9 | ... | 0.13+-0.06 | ... | -2.42+-0.06 | 0.13+-0.06 | 1.51+-0.06 | V II |
| Cr I | 7 | ... | -0.05+-0.09 | ... | -2.60+-0.09 | -0.05+-0.09 | 3.04+-0.09 | Cr I |
| Cr II | 20 | ... | 0.01+-0.06 | ... | -2.54+-0.06 | 0.01+-0.06 | 3.10+-0.06 | Cr II |
| Mn I | 3 | ... | -0.57+-0.01 | ... | -3.12+-0.01 | -0.57+-0.01 | 2.31+-0.01 | Mn I |
| Mn II | 4 | ... | -0.34+-0.04 | ... | -2.89+-0.04 | -0.34+-0.04 | 2.54+-0.04 | Mn II |
| Fe | N/A | -2.55 | ... | ... | -2.55 | ... | 4.95 | Fe |
| Fe I | 154 | -2.59+-0.1 | ... | ... | -2.59+-0.1 | ... | 4.91+-0.1 | Fe I |
| Fe II | 20 | -2.51+-0.09 | ... | ... | -2.51+-0.09 | ... | 4.99+-0.09 | Fe II |
| Co I | 27 | ... | 0.18+-0.08 | ... | -2.37+-0.08 | 0.18+-0.08 | 2.62+-0.08 | Co I |
| Ni I | 41 | ... | -0.05+-0.07 | ... | -2.60+-0.07 | -0.05+-0.07 | 3.62+-0.07 | Ni I |
| Cu I | 2 | ... | -0.69+-0.01 | ... | -3.24+-0.01 | -0.69+-0.01 | 0.95+-0.01 | Cu I |
| Zn I | 3 | ... | 0.31+-0.07 | ... | -2.24+-0.07 | 0.31+-0.07 | 2.32+-0.07 | Zn I |
Position
| Right Ascension : | Declination : | 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 | 42000 | 106 | N/A | N/A |