  In this paper, we study the entire radial solutions of the self-dual
equations arising from the relativistic SU(3) Chern-Simons model proposed by
Kao-Lee and Dunne. Understanding the structure of entire radial solutions is
one of fundamental issues for the system of nonlinear equations. In this paper,
we prove any entire radial solutions must be one of topological,
non-topological and mixed type solutions, and completely classify the
asymptotic behaviors at infinity of these solutions. Even for radial solutions,
this classification has remained an open problem for many years. As an
application of this classification, we prove that the two components u and v
have intersection at most finite times.
