Solutions to the general classical Coulomb three-body problem in the f
orm of rigid-rotator and fixed-shape configurations are studied. In th
e collinear case, some necessary and/or sufficient conditions for the
existence of the so-called charge-symmetrical, (-)(+)(-), and charge-a
symmetrical, (-)(-)(+), configurations are stated. These conditions in
volve relations between the geometrical and dynamical parameters of th
e system under study. The impossibility of the existence of a planar C
oulombic rigid rotator is demonstrated. In the two-dimensional case, f
ixed-shape solutions are studied analytically, and it is shown that, i
n the three-dimensional case, only fixed-shape solutions involving a t
riple collision and a static case are possible. Finally, some numerica
l experimentation, mostly based upon theoretical predictions of the wo
rk, is performed, and new bound (although unstable) rotating-oscillati
ng orbits for systems such as the positronium negative ion and helium
are found.