A new tool for the investigation of (2 + 1)-dimensional gravity is pro
posed. It is shown that in a stationary (2 + 1)-dimensional space-time
, the eigenvectors of the covariant derivative of the timelike Killing
vector form a rigid structure, the principal Killing triad. Two of th
e triad vectors are null, and in many respects they play the role simi
lar to the principal null directions in the algebraically special 4D s
pace-times. It is demonstrated that the principal Killing triad can be
efficiently used for classification and study of stationary 2 + 1 spa
ce-times. One of the most interesting applications is a study of minim
al surfaces in a stationary space-time. A principal Killing surface is
defined as a surface formed by Killing trajectories passing through a
null ray, which is tangent to one of the null vectors of the principa
l Killing triad. We prove that a principal Killing surface is minimal
if and only if the corresponding null vector is geodesic. Furthermore,
we prove that if the (2 + 1)-dimensional space-time contains a static
limit, then the only regular stationary timelike minimal 2-surfaces t
hat cross the static limit, are the minimal principal Killing surfaces
. A timelike minimal surface is a solution to the Nambu-Goto equations
of motion and hence it describes a cosmic string configuration. A sta
tionary string interacting with a (2 + 1)-dimensional rotating black h
ole is discussed in detail.