Abstract
-5 for which the theory is applicable. The variable energy debt parameter Ep used in computing the second order perturbation theory potential is chosen to be consistent with the long range dispersion interaction constant C6 computed using the f-values from Kurucz. © ESO 2005.
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Barklem, P. S., & Aspelund-Johansson, J. (2005). The broadening of Fe II lines by neutral hydrogen collisions. Astronomy and Astrophysics, 435(1), 373–377. https://doi.org/10.1051/0004-6361:20042469
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