Masses and widths of the charmed axial-vector mesons , , , and are calculated nonperturbatively in the Resonance-Spectrum-Expansion model, by coupling various open and closed meson-meson channels to the bare () and states. The coupling to two-meson channels dynamically mixes and lifts the mass degeneracy of the spectroscopic and states, as an alternative to the usual spin-orbit splitting. Of the two resulting -matrix poles in either case, one stays very close to the energy of the bare state, as a quasi-bound state in the continuum, whereas the other shifts considerably. This is in agreement with the experimental observation that the and have much smaller widths than one would naively expect. The whole pattern of masses and widths of the axial-vector charmed mesons can thus be quite well reproduced with only two free parameters, one of which being already strongly constrained by previous model calculations. Finally, predictions for pole positions of radially excited axial-vector charmed mesons are presented.

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