Physical conditions in CaFe interstellar clouds

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Gnacinski, P.; Krogulec, M.;
(2007)

Interstellar clouds that exhibit strong Ca I and Fe I lines were called CaFe clouds. The ionisation equilibrium equations were used to model the column densities of Ca II, Ca I, K I, Na I, Fe I and Ti II in CaFe clouds. The chemical composition of CaFe clouds is that of... View more
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