A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2007; you can also visit the original URL.
The file type is
Line Intensities and Molecular Opacities of the FeHF4Δi–X4ΔiTransition
We calculate new line lists and opacities for the F^4Δ_i-X^4Δ_i transition of FeH. The 0-0 band of this transition is responsible for the Wing-Ford band seen in M-type stars, sunspots and brown dwarfs. The new Einstein A values for each line are based on a high level ab initio calculation of the electronic transition dipole moment. The necessary rotational line strength factors (Hönl-London factors) are derived for both the Hund's case (a) and (b) coupling limits. A new set of spectroscopicdoi:10.1086/376791 fatcat:gk3sgp5md5copnrlhezwd4ab2u