We extend a recent computation of the dependence of the free energy, F, on
the non-commutative scale theta to theories with very different UV sensitiv
ity. The temperature dependence of F strongly suggests that a reduced numbe
r of degrees of freedom contributes to the free energy in the non-planar se
ctor, F-np, at high temperature. This phenomenon seems generic, independent
of the UV sensitivity, and can be traced to modes whose thermal wavelength
s become smaller than the noncommutativity scale. The temperature dependenc
e of F-np can then be calculated at high temperature using classical statis
tical mechanics, without encountering a UV catastrophe even in large number
of dimensions. This result is a telltale sign of the low number of degrees
of freedom contributing to F in the non-planar sector at high temperature.
Such behavior is in marked contrast to what would happen in a field theory
with a random set of higher derivative interactions.