BD-4_3208
taken from 2 paper(s):
/M.Bergemann et al.(2010)/
/M.Bergemann and G. Cescutti(2010)/

M.Bergemann et al.,MNRAS, 401, 1334, 2010 (A0225,ADS)
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 |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | N/A | N/A | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
M.Bergemann et al.,AAP, 522, A9, 2010 (A0237,ADS)
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 |
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 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |