Towards the solution of the λ Bootis problem

Having analysed the accretion‐based model of the dust–gas separation, which is regarded to be the most promising for the explanation of the anomalous properties of λ Bootis‐type stars, we can conclude that: (i) for any reasonable density profiles of the shell, dust grains appear to be decoupled from the gaseous background within the region where the temperature drops to a value that is less than the condensation temperature of heavy elements such as Mg, Ca, Fe, etc; (ii) most likely, in the shell of λ Bootis‐type stars only small dust particles (of less than ≈10 −6  cm in size) can be created; (iii) significant alteration of the initial atmospheric chemical composition can take place in the case when the density in the shell changes as ∼ r −2 .