  The present work deals with the dynamics of radiating star which is
considered to be expansion free cylindrical symmetric dust dissipative fluids.
Several treatments are adopted for the description of geometrical and physical
features of such stars. Firstly, it is shown that, the dynamical star does not
permit the streaming out limit and diffusion approximation and also proved that
acceleration and dissipation are necessary for its dynamical evolution. It has
also shown that, a static expansion free cylinder must be non-radiating.
Secondly, the existence of cavity model and self-similar solution for the such
dynamical star are also investigated.
