http://arxiv.org/abs/1812.11338
The evolution of close binary stars in mass asymmetry (transfer) coordinate is considered. The conditions for the formation of stable symmetric binary stars are analyzed. The role of symmetrization of asymmetric binary star in the transformation of potential energy into internal energy of star and the release of a large amount of energy is revealed.
V. Sargsyan, H. Lenske, G. Adamian, et. al.
Tue, 1 Jan 19
34/55
Comments: 21 pages, 7 figures