Generation of gravitational waves. III. derivation of bremsstrahlung formulae

Formulae are derived describing the gravitational waves produced by a stellar encounter of the following type: The two stars have stationary (i.e., nonpulsating), nearly Newtonian structures with arbitrary relative masses; they fly past each other with an arbitrary relative velocity; and their impact parameter is sufficiently large that they gravitationally deflect each other through an angle small compared to 900