  Static and uniformly rotating, cold and hot white dwarfs are investigated
both in Newtonian gravity and general theory of relativity, employing the
well-known Chandrasekhar equation of state. The mass-radius, mass-central
density, radius-central density etc relations of stable white dwarfs with
$\mu=A/Z=2$ and $\mu=56/26$ (where $A$ is the average atomic weight and $Z$ is
the atomic charge) are constructed for different temperatures. It is shown that
near the maximum mass the mass of hot rotating white dwarfs is slightly less
than for cold rotating white dwarfs, though for static white dwarfs the
situation is opposite.
