
doi: 10.1086/129524
A study of 51 main-sequence A to G stars shows that microturbulent velocities derived using the Kiel absolute f-values for Fe I are generally smaller than those determined with the Corliss and Warner f-values. Mso, in this spectral range excitation temperatures for Fe I come out to be higher by about - 0. in 0. Key words: microturbulence - oscillator strengths - Fe I f-values
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