In the early 1980s, our understanding of binary star evolution based on the pioneer work by Paczynski (1971), Tutukov and Yungelson (1973), van den Heuvel and Heise (1972), allowed us to construct a general evolutionary scenario which successfully explained the genesis of well-studied normal stars and offered potential explanation for new X-ray sources discovered in space experiments. It was recognized then that the evolution of binary systems looks like a branching genealogical tree whose nodes include important physical processes, such as the mass exchange between binary components, the common envelope stage (CE), loss of orbital angular momentum at the expense of gravitational wave emission and the magnetic stellar wind, etc.
On the other hand, it was clear that dramatic new processes should occur after a compact star (white dwarf (WD), neutron star (NS) or black hole (BH)) has been formed in a binary system. Taking account of these processes was especially important in the cases of WD and NS as they can have strong magnetic fields and rotate rapidly. Here, we come across a new phenomenon in stellar evolution - the evolution of gravitating magnetic compact stars (gravimagnetic rotators). The original idea goes back to pioneer work by V.F. Schwartzman (Schwartzman 1970a, 1971)[173, 176], Illarionov and Sunyaev (1975), Bisnovatyi-Kogan and Komberg (1975), Shakura (1975), Wickramasinghe and Whelan (1975), Lipunov and Shakura (1976), Savonije and van den Heuvel (1977), and Lipunov (1982a), and means that astrophysical manifestations of the magnetized compact star are mainly determined by its interaction with the surrounding plasma by means of two types of physical fields: electromagnetic and gravitational, and the evolution itself represents a gradual change of the character of this interaction. The universality of such an approach is not only its ability to explain apparently such different objects as radiopulsars, X-ray pulsars, X-ray bursters, cataclysmic variables, polars, transient X-ray sources, etc., but also its ability to predict completely new and still undiscoverd objects.
Therefore, the realistic treatment of binary star evolution must include both types of evolution: the nuclear evolution for the normal stars, and the rotational evolution for the compact magnetized stars. The last fact complicates the evolutionary tree to such a point that the need for a special numerical tool for studying binary evolution (the Scenario Machine), analysis of the observed picture and approval of the evolutionary scenarios becomes quite obvious (Kornilov and Lipunov, 1983a,b)[85, 86]. Now it consists of a large numerical code that incorporates the crucial physical processes in binary systems and takes into account:
The history of the Scenario Machine can be briefly summarized as follows.
Apart from giving an explanation for the known evolutionary stages of binary systems, this code proved to be a powerful tool for studying evolutionary links between different binary star populations (Lipunov, 1994). The results obtained with the Scenario Machine include the following.
Many important physical effects were shown to follow from the modern evolutionary scenario, among which are those listed below