  We discuss near-Hagedorn string thermodynamics in general spacetimes using
the formalism of the thermal scalar. Building upon earlier work by Horowitz and
Polchinski, we relate several properties of the thermal scalar field theory
(i.e. the stress tensor and U(1) charge) to properties of the highly excited or
near-Hagedorn string gas. We apply the formulas on several examples. We find
the pressureless near-Hagedorn string gas in flat space and a non-vanishing
(angular) string charge in $AdS_3$. We also find the thermal stress tensor for
the highly excited string gas in Rindler space.
