The interaction between convection and pulsation
allows access to the physics of convection by detailed
studies of their pulsation properties. Both high precision
data and numerical simulations of the stars are tools
which allow a better understanding of these processes.
In this talk I present applications of the ANTARES
simulation code used to study the convection-pulsation
interaction, chiefly of p-modes in main sequence stars,
though also results on other objects will be considered.
Investigations of the so-called near-surface effect,
mode damping, and overshooting will be considered.
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