  The present article reports on the second tool of a custom-built toolkit
intended to train astronomers into simulating and visualizing the composite 3D
structure of winds from hot close double stars by implementing a technique
which is similar to multi-directional medical tomography. The flagships of the
toolkit are the Spectrum Analyzer and Animator (SA 2 ) and the Binary 3D
Renderer (B3dR). Following application of the first tool, SA 2 as detailed in
paper I, the composite wind structure of the binary has been recovered and the
B3dR is subsequently employed to visualize the results and simulate the
revolution of the entire system (stars, winds and wind-interaction effects)
around the common centre of mass. The B3dR thus repackages the end product of a
lengthy physical modeling process to generate realistic multimedia content and
enable the presentation of the 3D system from the point of view of an observer
on Earth as well as from any other observer location in the Galaxy.
