  We consider an Einstein-Hilbert-Dilaton action for gravity coupled to various
types of Abelian and non-Abelian gauge fields in a spatially finite system.
These include Yang-Mills fields and Abelian gauge fields with three and
four-form field strengths. We obtain various quasilocal quantities associated
with these fields, including their energy and angular momentum, and develop
methods for calculating conserved charges when a solution possesses sufficient
symmetry. For stationary black holes, we find an expression for the entropy
from the micro-canonical form of the action. We also find a form of the first
law of black hole thermodynamics for black holes with the gauge fields of the
type considered here.
