The World Wide Web version provides the opportunity to construct an evolutionary track with all important parameters determined by the user at will from a broad range of available values.
Figure: Part of the table for the defauly output.
Some of the most unclear branches of the scenario can also be determined by the user. They include: the type of mass-loss of normal star, the lewel of conservativeness of the matter captured by the compact companion, the upper limit of the accretion rate at the CE stage by the compact object, switching of the accretion-induced magnetic field decay, etc.
Below we describe briefly how to handle the code, what the WWW-pages contain and how the results are presented.
Figure: Graphical diagram for the default output