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The mass transfer is typically modelled using two film theory.
We concluded that intraparticle mass transfer is negligibly small.
The increased mass transfer is affected by liquid cross flow.
The limitation due to mass transfer is negligible.
The case of mass transfer is examined in detail.
Interphase mass transfer is simulated using the film model.
This suggests that mass transfer is the rate-determining step.
The influence of pulsation on the mass transfer is studied.
A model of gas liquid mass transfer is also developed.
If the donor star stays approximately within its Roche lobe, mass transfer is dynamically stable.
These studies have shown that (initially) the mass transfer is episodic.
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