Fig. 23
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Kinetic abundances of aluminium-bearing species in the post-shock gas at 1 R⋆ of the pulsating SRV model as a function of pulsation phase, Φ. Dashed lines show the abundances when the photodissociation is excluded.Upper panel: initial abundances given by chemical equilibrium (TE). Lower panel: initial abundances corresponding to a pure atomic gas composition.
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